The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light distribution appears diffuse, lacking prominent spiral arm structures or a distinct bar. There is a subtle color gradient visible, with a slightly bluer hue in the outer regions compared to the more central area, which appears relatively redder. The overall appearance suggests a spheroid-dominated galaxy, possibly an elliptical or S0 type, at a moderate distance. There is no obvious evidence of ongoing major mergers or strong tidal disturbances; however, subtle asymmetries cannot be entirely ruled out given the resolution. The apparent size is relatively compact. The redder core relative to the bluer edges may indicate a difference in stellar population or dust distribution.
