The galaxy presents as a predominantly smooth, elliptical object. It exhibits a high degree of central concentration, with luminosity decreasing gradually towards the outer edges. The shape appears nearly circular. There is no obvious spiral arm structure or prominent dust lane visible. There are no signs of any ongoing major merger events, but a slight asymmetry in the outer isophotes may indicate a minor interaction or past disturbance. The color profile appears fairly uniform across the galaxy, suggesting an older stellar population dominating its composition. The overall color is mildly red, which supports the hypothesis of an older population. There is a lack of distinct blue star-forming regions or HII complexes visible in the image, this supports the idea of a relatively low star formation rate within the galaxy.