The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, with a gradual decrease in luminosity moving outwards. There is a lack of distinct spiral arm structures. The color profile suggests a primarily older stellar population, as indicated by the redder hues in the image. Some very minor distortions are potentially visible. There is no clear evidence of ongoing major merger activity, though some minor interactions cannot be entirely ruled out. It is approximately circular in shape.