The galaxy presents a generally smooth, elliptical morphology. The central bulge is prominent, displaying a concentrated luminosity profile that decreases gradually towards the outer regions. The color appears yellowish, suggesting a stellar population dominated by older, redder stars. There is minimal evidence of spiral arm structures or significant dust lanes. The galaxy exhibits a slight elongation, deviating marginally from a perfectly circular shape. There is no obvious sign of any significant ongoing mergers or tidal disturbances. The overall appearance indicates a relatively quiescent system with limited current star formation.
