The galaxy presents a generally smooth morphology, appearing elliptical in shape with a relatively high degree of symmetry. It is elongated, displaying an aspect ratio indicative of a galaxy that is either intrinsically cigar-shaped or an elliptical galaxy viewed at an angle.

The color profile is dominated by a yellowish-orange hue concentrated towards the central region, suggesting an older stellar population and a reduced rate of recent star formation activity. The outer regions exhibit a fainter, slightly bluer tint, potentially indicating the presence of a younger stellar population, albeit less prominent compared to the core.

There is no distinct spiral arm structure or evidence of a well-defined disk. No tidal tails or other obvious signs of a major recent merger are apparent, though there may be some minor disturbances in the outer halo. The galaxy appears to be a relatively isolated system, showing no strong signs of interaction with neighboring galaxies.
