This galaxy presents as a relatively smooth, elliptical structure. Its overall shape is elongated, but not highly cigar-shaped, and the light distribution suggests a centrally concentrated spheroid.

The core of the galaxy exhibits a distinct reddish-yellow hue, possibly indicating an older stellar population. Fainter, bluer light is observed in the outer regions, suggesting the potential presence of younger, hotter stars and/or some ongoing star formation activity, although this is not immediately apparent from the image.

There's a subtle asymmetry in the outer regions of the galaxy, hinting at the possibility of minor disturbances. These disturbances do not appear to be indicative of a major merger event, but they suggest the galaxy may have undergone some interaction in its past.
