The galaxy exhibits an elliptical morphology, appearing elongated with a cigar shape. The central region presents a smooth, diffused light distribution, suggestive of an older stellar population. There is evidence of a possible disk-like structure, though it is not clearly defined. A slight blue color in the outskirts may indicate some degree of recent star formation, though the overall star formation rate is low. There are no signs of major mergers or significant tidal disturbances; however, there is a minor irregularity or disturbance on one side. The galaxy exhibits relatively low mass compared to other galaxies, and is an intermediate luminosity galaxy. 
