The galaxy presents as a moderately bright, elliptical-shaped object with a relatively smooth texture. The central region exhibits a concentrated luminosity, suggesting a significant stellar population density, potentially an older population. There is a slight color gradient from the core to the outer regions, with the central region appearing somewhat yellow/white and the outer edges exhibiting hints of blue and red. This may indicate a difference in stellar populations, with a potentially older population in the center and younger stars mixed in at the edges. The galaxy lacks any obvious spiral arm structure or significant dust lanes. There is no visually apparent ongoing major merging activity or strong tidal disturbances. There seems to be only minor interaction and is primarily a smooth galaxy. 
