This galaxy presents as a relatively smooth, round object. It appears to lack defined spiral arms or a prominent disk structure. The light is centrally concentrated, with a bright core that fades gradually toward the edges. The color profile suggests a population of older stars, indicated by the redder hue concentrated towards the center. There is little evidence of significant dust lanes or active star formation regions in this image. Overall, the galaxy exhibits characteristics consistent with an elliptical morphology, appearing largely undisturbed. There are hints of color variation at the outer edges that may indicate an accretion event, but more data would be needed to confirm.
