The galaxy exhibits an overall elliptical morphology with a relatively smooth light distribution. There is a concentration of light toward the center, exhibiting a bright, somewhat elongated core region. The galaxy appears reddish in color, suggesting an older stellar population with lower ongoing star formation. Faint blueish features are also present, particularly around the central bulge, indicating the presence of some younger, hotter stars. The overall structure appears slightly disturbed, indicating possible minor gravitational interactions or past merger events. The galaxy exhibits an elongated shape. The color gradient suggests the presence of a stellar population gradient, with redder, older stars dominating the central regions and potentially younger, bluer stars populating the outer regions.
