The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, with a gradual decrease in luminosity outwards. The color profile is generally consistent, showing a slightly redder hue, suggesting an older stellar population and a relatively low rate of ongoing star formation. There are no readily apparent spiral arms or distinct features indicative of active star-forming regions. The overall form suggests a relatively relaxed, evolved system without significant signs of recent mergers or major disturbances. Its shape appears close to circular.
