The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It appears largely elliptical in shape, exhibiting a high degree of roundness. There is no obvious presence of spiral arms or a prominent disk structure. The galaxy's color profile suggests a redder hue overall, indicative of an older stellar population.

There is little evidence of ongoing major mergers or significant tidal disturbances. Faint features, possibly related to minor interactions or internal structures, may be present but are not distinctly resolved in this image. Overall, this galaxy appears to be a relatively undisturbed, passively evolving system.
