The galaxy appears as a centrally concentrated object with a smooth morphology, lacking prominent spiral arms or a distinct bar structure. There is an extension on the western side of the galaxy. The color profile suggests a relatively homogenous stellar population. The galaxy exhibits a moderate redshift, indicating that it is at an intermediate cosmological distance. There is no strong evidence of ongoing major mergers or significant tidal disturbances. The galaxy is estimated to be of considerable mass, implying a mature system. Overall, the galaxy appears to be an elliptical galaxy.
