The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish-orange hue, indicative of an older stellar population. Moving outward from the core, the luminosity gradually decreases into a fainter, diffuse halo. This outer region appears slightly bluer in color, suggesting the presence of younger stars, or at least a lower concentration of older stars relative to the core. The overall shape is elongated and somewhat cigar-shaped, but not extremely so. There is no apparent evidence of significant disk structures or prominent spiral arms. No signs of ongoing major mergers or tidal disturbances are visible, though the presence of minor interactions cannot be ruled out based on this image alone. The galaxy is moderately luminous, indicating a substantial stellar mass.
