The galaxy presents as a slightly irregular, disk-dominated system, approximately 6 kpc in effective radius. The overall color index suggests a relatively evolved stellar population, with the central region appearing more concentrated and yellow.

There's evidence of some disruption or tidal features. The disk appears somewhat disturbed, possibly due to a minor interaction or recent merger. Some low-surface-brightness light extends beyond the main body of the galaxy, hinting at stellar streams or tidal tails. The color distribution indicates some ongoing star formation, albeit at a moderate level, primarily in the outer disk regions. No dust lanes are readily apparent. The galaxy is likely of significant mass, possessing a substantial bulge component and a well-defined disk.
