The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. There is little discernible evidence of spiral arms or significant dust lanes. The light distribution appears concentrated towards the center, gradually fading out towards the edges. The galaxy displays a yellowish-red hue, suggesting a population of older stars and lower rates of star formation. There are no obvious signs of a major merger event or significant tidal disturbances affecting its overall morphology, though subtle disturbances cannot be ruled out. The shape appears to be somewhere between round and elongated.
