The galaxy presents as a smooth, elliptical form with a concentrated central bulge. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The light profile exhibits a relatively even distribution, fading gradually from the core outwards. The galaxy appears to be slightly elongated, exhibiting a mild cigar shape. There is no visual evidence of ongoing major merging activity or significant tidal disturbances affecting its morphology. The color index suggests a population of older stars.
