The galaxy presents as a relatively compact elliptical system. It exhibits a smooth, somewhat rounded morphology with minimal discernible internal structure. The light distribution appears centrally concentrated, indicative of a dominant bulge component. There's no distinct spiral arm structure or dust lanes visible. The overall color suggests an older stellar population, with a yellow-red hue indicating lower levels of ongoing star formation. There may be minor disturbances, but no strong signs of a major merger or interaction with another galaxy are seen.
