The galaxy appears to be a spiral type, exhibiting a faint disk-like structure. Although there are no defined spiral arms visible. The galactic bulge is subtle. Its stellar population seems relatively mixed, with a range of colors suggesting a diversity of stellar ages, though dominated by older stars in the central regions. There may be a slight disturbance indicating a possible minor interaction or merger in the past. The outskirts of the galaxy appear somewhat diffuse. The overall structure suggests a galaxy in a relatively quiescent state.
