The galaxy presents a generally smooth morphology, with a high degree of central concentration of light. It exhibits an elliptical shape, appearing neither perfectly round nor highly elongated. The central region displays a bright, yellowish-white hue indicative of an older stellar population. Fainter, somewhat diffuse extensions are visible along the major axis, suggesting the possible presence of a disk component or tidal features resulting from a past or ongoing interaction. There are some signs of disturbances. The light is somewhat asymmetric. The spiral arms if present are tightly wound. There is a slight variation in colour across the galaxy, hinting at differences in the stellar populations and dust content within different regions.
