The galaxy presents as a relatively smooth, centrally concentrated object. It appears to exhibit a slight elongation, deviating marginally from a perfect circle. The color profile suggests a dominant population of older stars, indicated by the yellowish-red hue concentrated in the central bulge. There is a faint disk structure surrounding the core, with hints of bluer colors that could indicate regions of more recent, although subdued, star formation. No significant spiral arm structure or tidal features are discernible, suggesting that the galaxy is unlikely to be undergoing major merger activity. The outer regions of the galaxy appear diffuse, gradually fading into the background sky.
