The galaxy presents as a moderately luminous, elliptical form with a smooth, diffuse light profile. The core region appears to exhibit a reddish hue, suggesting a potentially older stellar population or dust obscuration. The outer regions display a subtle, greenish tint. The overall shape is somewhat elongated, trending toward a cigar-like morphology. There appears to be no strong evidence of significant spiral arm structure or ongoing major merging events. There is a minor disturbance to the left of the galaxy. The galaxy is a relatively isolated object.
