The galaxy presents as a relatively smooth, centrally concentrated object. There is some indication of deviation from a perfectly circular shape, perhaps slightly elliptical. The color profile suggests a dominant population of older stars, with a concentration of redder hues in the central region, indicative of an evolved stellar population. There is a subtle hint of bluer light in the outer regions, potentially indicating ongoing star formation. There is some visual evidence of a minor merger event, but it is hard to discern the extent of the impact on the overall galactic structure.
