The galaxy presents as a moderately inclined, disk-shaped system. Its overall form appears relatively smooth and lacking in prominent spiral arm structures. The central bulge is not particularly pronounced, suggesting a later type classification. The color profile indicates a somewhat evolved stellar population, leaning towards redder hues, although some bluer regions are subtly present, possibly indicative of localized star formation. There might be minor tidal disturbances around the galaxy, but it appears to be a stable non-merging system. The overall impression is of a lenticular or early-type spiral galaxy at a significant distance.
