The galaxy appears as a centrally concentrated object with a relatively smooth light distribution. The morphology suggests a lack of significant spiral arm structure. The color profile is subtly reddish, indicating a potentially older stellar population and/or the presence of dust. The galaxy exhibits a generally elliptical shape with a tendency towards being in between round and elongated. No major disturbances or merging features are readily apparent, suggesting it is relatively isolated and undisturbed. The overall impression is that of a fairly evolved, relatively quiescent system.
