The galaxy presents as a centrally concentrated object with a relatively smooth morphology. The primary color of the core appears yellowish-white, indicating a likely older stellar population dominating this region. A faint, diffuse halo of bluish light surrounds the core, suggesting the presence of a younger stellar population with ongoing or recent star formation activity. There are hints of possible spiral arm structure or tidal disturbances, but the resolution is insufficient to definitively confirm either. The overall shape is elliptical or nearly round, and the lack of obvious dust lanes implies the galaxy is relatively face-on. No companion galaxies are immediately apparent within the visual proximity that would be considered a major merger candidate, although minor disturbances cannot be ruled out.
