The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated morphology with a generally round shape. There are no visible spiral arms or distinct features indicative of a disk. The color profile suggests an older stellar population, exhibiting a redder hue overall. There is some evidence of a possible minor interaction or merger event in progress. A slight asymmetry is noted within the outer isophotes and possibly a faint tidal tail present extending from the galaxy. This object has a relatively low star formation rate. 
