The galaxy appears as a relatively smooth, elongated structure. The light distribution is centrally concentrated with a noticeable decrease in surface brightness towards the outer regions. There is a color gradient observable, with the central region displaying a yellowish-orange hue, suggestive of an older stellar population. The outer regions exhibit a bluer tint, potentially indicating the presence of younger, hotter stars, and ongoing star formation. There are no obvious signs of strong spiral arms or a prominent central bulge. The overall morphology suggests a late-type spiral or lenticular galaxy, viewed at a high inclination angle. Faint, diffuse extensions are possibly present along the major axis, hinting at a possible tidal interaction.
