The galaxy presents a generally smooth, elliptical morphology, though with noticeable deviations from perfect ellipticity. The core region exhibits a high surface brightness, with a concentration of light suggesting a dense stellar population. The galaxy's light profile is elongated, appearing cigar-shaped, with a major axis that is notably longer than its minor axis. There is an apparent minor disturbance or potential merging event. It is visibly separate from the core of the galaxy, but in close proximity. Overall, the galaxy gives the impression of a mature system, although with a rate of active star formation.
