The galaxy appears as a centrally concentrated object with a generally smooth light distribution. It displays a moderate ellipticity, leaning toward a cigar shape. No distinct spiral arm structures are visible, nor is there evidence of a prominent central bulge or bar. The color appears relatively uniform across the galaxy, suggesting an older stellar population with low levels of ongoing star formation. There are no obvious signs of recent major mergers or tidal disturbances in the immediate vicinity, although a slight asymmetry in the galaxy's profile might indicate minor interactions. The galaxy is relatively compact in size.
