This galaxy appears to be an elliptical type, displaying a smooth, diffuse morphology. It has a moderately elongated shape, suggesting a classification leaning towards an E4 or E5 on the Hubble scale. The core exhibits a higher concentration of light, likely indicative of an older stellar population. Fainter, bluer hues are present in the outer regions of the galaxy, which might suggest some younger stars or ongoing star formation. There is no obvious evidence of spiral arms or a distinct dust lane. The galaxy doesn't show any indications of recent major mergers or strong tidal disturbances; however, a slight asymmetry might hint at a past minor interaction. The galaxy has an intermediate size. Overall, this galaxy seems to be a relatively undisturbed elliptical, possibly in a stage of transitioning from active star formation to quiescence.
