The galaxy exhibits a generally elliptical morphology, appearing moderately smooth with some indications of faint, diffuse features. The central region displays a concentrated, bright, and slightly reddish-yellow hue, suggesting a population of older stars. The galaxy has a noticeable degree of elongation but not extreme. Fainter, more diffuse blue light emanates from the outer regions, hinting at possible ongoing, though limited, star formation activity. There is a suggestion of a minor disturbance in the overall structure, possibly resulting from a past or ongoing interaction with a smaller companion object. Overall, the galaxy appears to be a relatively massive system at a moderate redshift.
