The galaxy appears as a single, slightly elongated object with a centrally concentrated light profile. The primary color is a yellowish-white hue, suggesting an older stellar population. There is a slightly more bluish region to the upper left. The overall structure is mostly smooth, with no apparent spiral arm features or distinct dust lanes. However, the slight asymmetry and the color variation suggest that this galaxy is involved in a merger. A significant fraction of the light appears to be centrally concentrated within a relatively compact region, but some light is also distributed less intensely in the surrounding region. There may be evidence of minor tidal disturbances or distortions within the extended halo region surrounding the primary galaxy.
