The galaxy presents as a relatively smooth, centrally concentrated object with a notable reddish-yellow hue. The morphology appears elliptical or spheroidal, with no distinct spiral arms or bar structures visible. The light profile suggests a high degree of central concentration, with the luminosity decreasing gradually towards the outer regions. There are no prominent tidal features or obvious signs of ongoing major mergers, although some subtle asymmetry or minor disturbances cannot be ruled out. The overall color indicates a stellar population dominated by older, redder stars, suggesting a relatively low rate of ongoing star formation. The galaxy's size is moderately compact.
