The galaxy presents as a fairly smooth, elliptical-like structure, exhibiting a somewhat round morphology. There is little to no indication of prominent spiral arms or a well-defined disk. The light profile appears relatively concentrated, with the highest intensity near the center, gradually fading outwards. The color of the galaxy is predominantly yellowish, suggesting a population of older stars, and a relatively low rate of current star formation. There is some evidence of possible minor disturbance in the galaxy's morphology, perhaps indicative of a past minor merger or interaction, but no major distortions or tidal features are visible.
