This galaxy appears to be a relatively smooth, elliptical system, exhibiting a concentrated central bulge that dominates the overall structure. The galaxy displays a yellow-red hue, suggesting an older stellar population with fewer ongoing star formation regions. The outskirts of the galaxy appear diffuse and fading, with a noticeable flattening along the major axis. There is evidence of minor disturbances or irregularities present in the morphology, possibly indicating interactions or past merger events. A faint disk structure may be present as well.
