The galaxy presents as a relatively smooth, elongated structure. The orientation is close to edge-on, with a clear major axis. The central region exhibits a brighter, more concentrated luminosity, suggestive of a central bulge. The bulge appears rounded. The disk component is also smooth and does not show prominent spiral arm features or significant dust lanes, at least in the visible spectrum, contributing to the overall smooth appearance. There is no indication of tidal tails or strong distortions to indicate a major merger event, but there is slight asymmetry. The galaxy's color suggests a generally older stellar population, with a possible contribution from dust extinction. The size appears relatively moderate. Overall, the galaxy seems to be a fairly quiescent, edge-on disk galaxy.
