The galaxy presents a generally smooth and elliptical morphology. It has a relatively high degree of central concentration with a bright, somewhat diffuse core. Moving outward from the core, there's a gradual decrease in luminosity, exhibiting a smooth transition into the outer regions of the galaxy. The overall shape is elongated, appearing somewhat cigar-shaped. There is no strong evidence of spiral arm structures or significant dust lanes visible. The color profile is relatively uniform, with a slight bluish tint that could imply some ongoing, though limited, star formation. No major merging activity or tidal disturbances are clearly apparent in the immediate vicinity of the galaxy.
