The galaxy presents as a relatively smooth, centrally concentrated object, with an apparent slight elongation. The core region exhibits a bright, diffuse glow, suggestive of a significant stellar population density. There is a subtle, extended halo surrounding the main body. A potential feature or disturbance appears to the upper left. The color profile indicates a population with a range of ages, with the central regions possibly composed of older stars while the slightly bluer hue could indicate a population with more recent star formation. It does not appear to be experiencing a major merger event, but a slight asymmetry or distortion implies a possible minor gravitational interaction or past merger.
