This galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central region. The galaxy exhibits a fairly high degree of circular symmetry, lacking any obvious signs of significant tidal disturbances or ongoing mergers, though the limited resolution makes subtle features difficult to discern. The color profile suggests a population of older stars, as indicated by the overall yellowish hue, with the central region appearing somewhat brighter and potentially slightly bluer than the outer regions. There is very little evidence of distinct spiral arms or pronounced dust lanes. Overall, the galaxy appears to be a relatively quiescent system.
