The galaxy presents as a generally smooth and rounded structure. A concentrated central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy show a more diffuse, bluish tint, potentially indicative of younger, hotter stars. The lack of well-defined spiral arms or a distinct disk suggests a classification towards the elliptical or lenticular end of the Hubble sequence. There's no obvious evidence of ongoing major mergers or significant tidal disturbances in this image, although a minor disturbance cannot be ruled out. Star formation appears to be relatively low. Overall, it's a fairly isolated, quiescent galaxy.
