The galaxy presents as a faint, elongated structure with a noticeable central bulge. It appears relatively smooth overall, with minimal discernible spiral arm structure. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region, transitioning subtly to bluer tones at the edges. The galaxy exhibits a slight degree of asymmetry, possibly indicative of a minor tidal interaction or internal disruption. It is a medium sized galaxy with no apparent active galactic nuclei. The mass is on the high end, but the star formation rate is low.
