The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. It presents a concentrated central bulge region that gradually fades into the outer regions. The color profile suggests an older stellar population, with a yellow-orange hue dominating the galaxy's light output. There is little evidence of active star formation, as indicated by the lack of prominent blue regions associated with young, hot stars. The galaxy displays a relatively regular, near-spherical shape, with a slight elongation. There are no obvious signs of recent or ongoing major mergers or tidal disturbances, though there is a possible minor interaction or disturbance that is difficult to determine. Overall, the galaxy seems to be a well-formed, evolved system likely residing in a relatively quiescent environment.
