The galaxy presents as a slightly elongated, disk-shaped structure with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Surrounding the bulge, the disk appears bluer, potentially indicating ongoing star formation. The outer edges of the disk seem somewhat diffuse and indistinct, lacking sharp boundaries. There is a faint suggestion of spiral arm structure, though it is not sharply defined in this image. The galaxy's overall morphology leans towards a relatively smooth structure with some subtle features. It appears relatively isolated, with no signs of major interactions or mergers, although there may be some minor tidal disturbances present.
