The galaxy presents as an object with an apparent elliptical morphology, though deviation from perfect elliptical symmetry is noted. The light distribution is relatively smooth, with no distinct spiral arm structures visible. A central bulge is present, exhibiting a higher surface brightness than the surrounding regions. There is an indication of a slight tidal disturbance or interaction, as evidenced by a subtle distortion of the outer isophotes, suggesting possible past or ongoing gravitational interaction with another galaxy. The galaxy's overall color appears moderately redder, suggesting a stellar population dominated by older, redder stars, but there seems to be some blue coloring in one region that might indicate the presence of younger stars. The galaxy displays a diffuse halo, which extends beyond the main body of the galaxy.
