This galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. It possesses a noticeable central bulge, appearing more luminous than its surrounding regions. The galaxy exhibits a yellowish hue, suggestive of a population of older stars. There is a subtle color gradient from the core outwards, perhaps indicating subtle variations in stellar populations. The lack of distinct spiral arms or prominent dust lanes, coupled with its smooth appearance, supports a classification as an elliptical or lenticular galaxy. There is no evidence of significant tidal disturbances or interactions with neighboring galaxies in the immediate vicinity, suggesting a relatively isolated system. The shape appears to be in between round and cigar shaped, trending closer to round. Possible minor disturbance, though the bulk of measurements suggest it is not merging. 
