The galaxy presents a mostly smooth morphology with a slight elongation, appearing somewhat cigar-shaped.  Its color profile indicates a generally older stellar population. A central, brighter bulge region shows a yellower hue.  The outer regions of the galaxy exhibit a bluer tint, suggesting the presence of some younger stars. However, these regions lack distinct spiral arm structures or prominent star-forming knots. The galaxy does not appear to be undergoing any major merging events or experiencing substantial gravitational disturbances. There are no prominent tidal tails or warped disk features visible.
