The galaxy presents an overall smooth morphology with a centrally concentrated brightness profile, suggesting a dominant bulge component. The shape is somewhat elliptical, not perfectly spherical. There is evidence of tidal disturbance or ongoing interaction, visible as a plume or tail-like extension emanating from the main body of the galaxy. This feature exhibits a redder color, possibly indicating older stellar populations. The core region appears yellowish, which might signify the presence of an intermediate-age stellar population. The overall color of the galaxy suggests a relatively evolved system, but there may still be some ongoing star formation. The galaxy is estimated to be a high mass object with likely very low star formation.