The galaxy appears as a relatively smooth, elliptical-like structure, displaying a concentrated central bulge. The overall color profile indicates a redder hue, suggesting a population of older stars. A subtle asymmetry or minor disturbance in the outer regions is weakly indicated. There is little evidence of strong ongoing star formation within the visible structure. The shape appears mostly round, lacking any cigar-shaped morphology. The galaxy's light distribution is centrally concentrated, with intensity gradually decreasing towards the outer edges.
