The galaxy presents a generally smooth morphology, with a somewhat elliptical shape. There is a strong central bulge which appears to be the brightest region of the galaxy. A faint, diffuse disk is seen extending outward from the central bulge, contributing to the overall elliptical appearance. The galaxy exhibits a redder color profile, suggesting an older stellar population with relatively little ongoing star formation. No distinct spiral arm structure is discernible. There is no evidence of any major mergers or significant tidal disturbances in the immediate vicinity.
