The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, with an observed aspect ratio that leans towards being somewhat rounded rather than elongated. The galaxy exhibits a prominent bulge component that dominates the overall luminosity profile. The color gradient suggests an older stellar population within the bulge region, as indicated by the redder hues. The outer regions of the galaxy show bluer colors, possibly indicating the presence of younger stars or some residual star formation, although this activity appears subdued. There is no evidence of a pronounced disk structure or spiral arms. We see no significant signs of ongoing major merger activity or strong tidal disturbances. There's very minor irregularity in the outer regions suggesting potential minor disturbances.
