The galaxy presents as a relatively smooth, elliptical-like structure. It is characterized by a concentrated central bulge that emits primarily yellow-orange light, suggesting a population of older stars. The light tapers off smoothly from the center, indicating a lack of prominent spiral arms or distinct features. The overall morphology leans towards a spheroid, appearing more rounded than elongated, although a slight elongation is visible. There is no visible evidence of tidal tails, merging activity, or strong dust lanes. The color suggests that star formation is either low or has largely ceased.
