The galaxy presents as a centrally concentrated, elliptical-shaped structure. The central region exhibits a bright, diffuse glow, possibly indicative of an older stellar population. The outer regions appear more elongated, fading into the background with a gradual decrease in luminosity. A slight color gradient is apparent, with the central region tending towards a redder hue and the outer regions showing a hint of bluer tones. The overall morphology suggests a relatively smooth distribution of light, with no prominent spiral arms or distinct dust lanes visible. There is a subtle asymmetry, with one side appearing slightly more extended than the other.
