The galaxy presents as a somewhat elliptical object. The galaxy exhibits a smooth morphology, appearing largely featureless without prominent spiral arms or a distinct central bulge. The color profile indicates the presence of both older stellar populations, inferred from the redder hue in the central regions, and younger, bluer stars, suggested by the blue tint around the edges. The object displays a high degree of circularity. No evidence of significant tidal disturbances or ongoing major mergers is apparent. Subtle irregularities in the outer regions hint at potential minor interactions or past accretion events.
