The galaxy presents a generally elliptical morphology, with a high degree of smoothness across its primary structure. The overall color profile suggests a relatively evolved stellar population, with a dominant yellowish-white hue concentrated toward the central regions. Fainter, bluer components appear sparsely distributed towards the periphery, hinting at ongoing, albeit subdued, star formation. A subtle distortion is visible along the galaxy's major axis, suggesting a possible interaction or minor disturbance. There may be a merging event, or perhaps the tail end of one. A clear spiral structure is not obviously apparent. The galaxy exhibits a moderate compactness, with its light concentrated within a radius that suggests a mass consistent with a typical galaxy.
