The galaxy presents a generally smooth morphology, with no prominent spiral arms or bar structures readily apparent. It appears elliptical, exhibiting a shape that is somewhat rounded. There is a slight elongation noticeable, but it does not approach a highly flattened or cigar-like appearance. 

Color gradients suggest some variation in stellar populations. The galaxy displays a noticeable core that is more luminous and compact, with a somewhat redder hue in comparison to the outer regions. This could indicate an older stellar population concentrated towards the center. The outer regions appear slightly bluer, possibly indicating the presence of younger, hotter stars, but the blue component is not substantial, suggesting that any ongoing star formation is not overwhelmingly dominant.

There are no obvious signs of major disturbances or ongoing mergers. The overall structure seems relaxed, without tidal tails or bridges that would be indicative of significant gravitational interactions with other galaxies. However, there might be some subtle asymmetry hinting at past minor interactions.
