The galaxy presents as a slightly elongated or cigar-shaped structure. A smooth, centrally concentrated bulge dominates the light profile, exhibiting a yellowish hue, indicative of an older stellar population. Surrounding the bulge is a more diffuse, bluer envelope. This envelope shows some subtle hints of disk-like structure, though without well-defined spiral arms. There might be some features, but it is hard to tell for sure. The galaxy doesn't appear to be undergoing any major merging activity or tidal disruption. 
