The galaxy appears as a centrally concentrated, smooth object with a moderate elliptical shape. The light distribution suggests a prominent bulge component. There is a gradient in the color profile, the core exhibiting a more yellow hue, and the outer regions gradually becoming redder. This could indicate an older stellar population dominating the central regions, with relatively less recent star formation activity in the central areas. The outer regions are faint and indistinct, and are not well resolved at this image scale. There is no apparent spiral structure or disk features visible. There is no evidence of any ongoing major merger events or tidal disturbances in the immediate vicinity of the galaxy. Overall, the galaxy displays characteristics consistent with an early-type galaxy or a massive spiral galaxy with a dominant bulge.
