The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a high degree of central concentration, with a bright core that diminishes in luminosity outwards. The overall color appears to be somewhat redder in hue, suggestive of an older stellar population with less ongoing star formation. There's no clear evidence of spiral arms or prominent disk features visible in this image, supporting the classification as an elliptical galaxy. Faint extensions or tidal features are not immediately apparent, although a minor disturbance cannot be entirely ruled out. The galaxy is generally rounded in appearance with a hint of an extended halo structure surrounding the central bulge. There are no obvious signs of a major merger or significant interaction with another galaxy.
