The galaxy appears to be a relatively smooth, centrally concentrated object. There is a noticeable color gradient from a yellowish core to a slightly bluer outer region. The light distribution is elliptical, with the galaxy appearing somewhat rounded rather than highly elongated. No obvious spiral arm structure or strong dust lanes are visible. The galaxy appears relatively isolated, with no strong signs of ongoing major merger activity or significant tidal disturbances, although there may be some minor disturbances visible. Based on the color distribution, the central region likely contains an older stellar population, while the bluer outskirts potentially indicate more recent star formation. The overall smooth appearance suggests the galaxy could be a lenticular or early-type spiral galaxy seen at a moderate redshift.
