The galaxy appears to be a relatively small, early-type galaxy. Its morphology is generally smooth and elliptical, exhibiting a centrally concentrated brightness profile with a gradual decline in luminosity towards the outer regions. There is little evidence of spiral arms or a prominent disk structure. The central bulge is prominent, showing a bright, concentrated core that likely hosts a supermassive black hole.

The color profile suggests a primarily older stellar population, as indicated by the relatively redder hues present within the galaxy. There is minimal evidence of significant ongoing star formation. The shape is mostly round with a mild, elongated shape. There is no noticeable sign of any major ongoing galaxy mergers or recent major disturbances. 
