The galaxy presents as a relatively bright object with a smooth, elliptical morphology. There is a noticeable lack of distinct spiral arm structure or prominent dust lanes. The light distribution appears centrally concentrated with a gradual decrease in surface brightness towards the outer edges. Color gradients suggest the presence of older stellar populations, with the central region possibly exhibiting a slightly redder hue. There are slight disturbances that are likely not a major merger. The absence of clear blue knots or HII regions implies a relatively low ongoing star formation rate. Overall, this galaxy appears to be an early-type galaxy with a considerable mass and modest star formation activity.
