The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a slightly elongated, but not highly distorted, shape. The light distribution suggests a bulge-dominated system, with a gradual decrease in brightness moving outwards from the core. There is no clear evidence of spiral arm structure or a distinct disk. The overall color is yellowish-white, indicating a relatively older stellar population. There appears to be minimal evidence of recent major merger activity, although some minor asymmetries cannot be entirely ruled out.
