The galaxy presents a generally elliptical morphology, with a high degree of central concentration. It exhibits a smooth light distribution, lacking distinct spiral arms or prominent dust lanes. The color profile suggests a population of older stars, with a yellowish-orange hue dominating the core and extending into the outer regions. There is some indication of a slight elongation, although the overall shape is predominantly round. A smaller, fainter object appears in close proximity to the primary galaxy, possibly interacting or representing a background galaxy along the same line of sight. There is no strong evidence of ongoing major star formation, and no tidal tails or other debris are apparent, suggesting a relatively undisturbed system.
