The galaxy presents as a slightly elongated, disk-like structure with a smooth, relatively featureless appearance. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus or bulge. A radial color gradient is present, with the central bulge displaying a yellowish hue, possibly indicative of an older stellar population. The outer regions of the galaxy appear fainter with bluer tones, potentially due to ongoing or recent star formation activity. The overall form approximates a spheroid, with a cigar-shaped morphology, but lacks any clear spiral arm structure or significant dust lanes. There's no obvious evidence of tidal disturbances or ongoing major mergers, although minor irregularities could potentially exist upon further analysis. Based on the apparent color and smooth morphology, this object could be classified as an early-type spiral galaxy with low-level star formation.
