The galaxy presents as a generally smooth, elliptical form, with a noticeable concentration of light toward the center. The core region appears yellowish-white, indicative of an older stellar population. Fainter, more diffuse light extends outwards from the central core, fading into the background. The overall color suggests a relatively low rate of ongoing star formation. There is no prominent disk structure or spiral arm features apparent in this image. The galaxy shows a slight elongation and there is no evidence of strong tidal disturbance or ongoing mergers, suggesting a relatively isolated evolutionary path.
