The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing nearly round but slightly elongated. The core region is bright and yellowish in color, indicating an older stellar population. Fainter, bluer hues surrounding the core suggest some ongoing star formation, although at a modest rate. There is no evidence of prominent spiral arms or a distinct disk structure, and there are no apparent signs of recent major merger events. Minor irregularities along the galaxy's edge might indicate a minor interaction with a satellite galaxy or tidal disturbances. Overall, the galaxy appears to be an intermediate-mass system with a mix of stellar populations and a moderate degree of star formation activity.
