The galaxy appears as a somewhat compact object. The central region exhibits a bright, concentrated luminosity, indicative of a possible active galactic nucleus or a dense stellar population. The galaxy's overall shape is roughly elliptical, showing hints of a disk-like structure. There are faint, asymmetric extensions or tidal features surrounding the central body, suggesting potential past interactions or ongoing minor disturbances. The color profile shows a blue-ish hue, particularly around the center, transitioning to a redder color toward the edges. This may indicate differing stellar populations, with younger, hotter stars concentrated centrally and older, cooler stars more prevalent in the outer regions. The light distribution appears relatively smooth, with minimal evidence of distinct spiral arm structures.
