The galaxy appears as a concentrated central region with a more diffuse surrounding structure. The core exhibits a yellowish hue, suggestive of an older stellar population. A slightly bluer, less concentrated region extends asymmetrically from the central core, potentially indicating ongoing star formation or a tidal feature. The overall shape appears somewhat rounded, although some irregularity is present. The outer regions of the galaxy fade into the background noise, making a precise determination of its boundaries difficult. The galaxy may be in the process of merging with another smaller galaxy, or may just be a normal galaxy that has a bar.
