The galaxy presents as an elongated, disk-like structure. It appears to be an edge-on or nearly edge-on spiral galaxy. A central bulge is visible, characterized by a concentrated, brighter region that gradually fades into the surrounding disk. The disk itself appears relatively smooth with little evidence of distinct spiral arm structures at this resolution. There is a slight asymmetry or warp noticeable along the major axis, suggesting possible gravitational interaction or past merger event, though no obvious companion galaxy is observed nearby in this field. The color gradient transitions from a slightly bluer hue in the outer regions to a redder hue towards the central bulge. The relative lack of prominent dust lanes suggests a relatively low dust content or a viewing angle that obscures their presence.
