The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears centrally condensed, with a gradual fading towards the edges. The galaxy exhibits a yellowish-orange hue in its central region, suggesting an older stellar population. The outskirts show a hint of a slightly bluer colour, potentially indicating the presence of some younger stars, but the dominant population appears to be older. There is a subtle asymmetry or possible distortion in the outer regions which might indicate a past minor interaction. The overall appearance suggests a relatively massive galaxy with a moderately low rate of star formation.
