The galaxy presents as a somewhat elliptical, relatively smooth structure. A bright, concentrated central bulge is evident, exhibiting a yellowish hue, potentially indicating an older stellar population. Moving outward from the core, there appears to be a gradual decrease in luminosity, forming a less defined disk. The outer regions display a faint greenish tint, which may be indicative of some ongoing, albeit low, star formation activity or a different stellar population compared to the central bulge. The galaxy exhibits an overall regular morphology, with no obvious signs of major tidal distortions or ongoing mergers. Subtle irregularities are observed in the disk area. The galaxy's color suggests that the central region is dominated by older stars and that newer star formation is predominantly occurring in a less concentrated disk.
