The galaxy presents as a relatively smooth object with a concentrated central region. The light profile appears to be dominated by an elliptical morphology, with a noticeable lack of spiral arm structure or prominent dust lanes. The color distribution indicates a slightly redder core, transitioning to a bluer halo or outer region. There may be some minor disturbances in the halo, but the galaxy's shape is predominantly undisturbed, suggesting the absence of a major merger event in recent history. The overall round appearance suggests that the viewing angle may be close to face-on. Based on the color properties, this galaxy is likely composed of an older stellar population in the core, with younger stars forming in the outer regions.
