The galaxy presents as a smooth, elliptical object with a concentrated central bulge and a more diffuse outer halo. The color profile exhibits a redder hue, suggesting an older stellar population with a lower rate of ongoing star formation. There are no prominent spiral arms or distinct features indicative of active star-forming regions. A slight asymmetry is observed in the outer regions, which may indicate minor gravitational interaction with another galaxy or past merger events. The galaxy is relatively compact in size, with an overall morphology that is classified as elliptical.
