The galaxy presents as an elliptical morphology, appearing elongated with a cigar-like shape. The light distribution suggests a relatively smooth profile. There is a concentration of light toward the center, indicating a defined nucleus or bulge. The overall color of the galaxy appears to be reddish-yellow, potentially indicating an older stellar population with less ongoing star formation. There is no obvious presence of spiral arms or dust lanes, further supporting the classification as an elliptical galaxy. The galaxy is isolated, with no indication of nearby interacting galaxies or major tidal disturbances. There is no discernible evidence of recent or ongoing major mergers.
