The galaxy presents as a slightly elongated, disk-shaped structure. Its orientation is close to edge-on relative to our line of sight, exhibiting a clear major axis. The galaxy appears relatively smooth and featureless, lacking prominent spiral arms or distinct dust lanes. There is a subtle color gradient visible, with a suggestion of a bluer hue towards the outer regions of the disk and a generally redder color toward the central bulge. Based on this, the galaxy is likely a late-type spiral or lenticular galaxy, potentially with a relatively low ongoing star formation rate. Evidence suggests it is not currently undergoing a major merger event, although some minor gravitational disturbance may be possible.
