The galaxy presents as a smooth, centrally concentrated elliptical galaxy with a notable lack of distinct spiral arm structures. The light profile appears very smooth, without any noticeable dust lanes or prominent features. The color is primarily a yellowish-red hue, suggestive of an older stellar population and a relatively low rate of recent star formation activity. The overall shape is somewhat flattened, but not to a degree that would classify it as lenticular. There is no evidence of ongoing major merger activity or significant tidal disturbances. The galaxy exhibits a high degree of central concentration, indicating the presence of a substantial bulge component.
