The galaxy presents as a lenticular or possibly an elliptical system, displaying a generally smooth, featureless morphology. It exhibits an elongated, cigar-like shape, with the major axis significantly exceeding the minor axis. The color gradient suggests a relatively uniform stellar population, with a yellow to slightly reddish hue, indicative of older stars and a dearth of ongoing star formation. There is a brighter central region, which could represent a galactic bulge. No spiral arms, dust lanes, or other distinct features are discernible, suggesting minimal recent interaction or merging events. The galaxy appears to be relatively isolated, showing no obvious signs of tidal distortion or nearby companion galaxies.
