The galaxy appears as a concentrated, relatively smooth, elliptical object. It has a bright, well-defined central region, likely a bulge, with a gradual decrease in luminosity toward its outer edges. The galaxy exhibits a yellowish-white hue, suggesting a stellar population dominated by older, redder stars, consistent with a low star formation rate. There is a slight asymmetry to the isophotes, which may indicate a weak tidal interaction or minor disturbance in its past. The overall structure suggests a galaxy that is nearing a state of quiescence. It is generally elliptical.
