This galaxy presents a roughly elliptical morphology, displaying a relatively smooth light distribution across its surface. The central region exhibits a higher concentration of luminosity, gradually decreasing towards the outer edges. A subtle color gradient is observed, with the core appearing slightly redder compared to the bluer hues visible in the extended halo. There are no readily discernible spiral arms or prominent dust lanes visible. The overall structure suggests a classification as an early-type galaxy, potentially an elliptical or lenticular galaxy, viewed at a moderate cosmological distance. There are no indications of major mergers, but a very faint asymmetry indicates it may have experienced a minor disturbance at some point.