The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region. There is little evidence of spiral arm structure or significant dust lanes. The overall morphology appears regular, showing no signs of major tidal disturbances or ongoing mergers, although a slight asymmetry cannot be entirely ruled out. The galaxy's round appearance indicates a relatively low inclination angle with respect to our line of sight. Based on the color and morphology, star formation appears to be suppressed.
