The galaxy appears as a smooth, centrally concentrated object with a relatively round morphology. It exhibits a yellowish-orange hue, indicative of a population of older stars. The galaxy's light profile suggests a possible elliptical galaxy, with little to no evidence of spiral arms or a prominent disk structure. There is a slight elongation, but the overall shape is closer to round than cigar-shaped. There does not appear to be any signs of ongoing major mergers or significant tidal disturbances. Based on the color, stellar mass, and morphology, star formation activity seems relatively low, but some moderate level is possible. 
