The galaxy presents as an elliptical morphology, elongated and approximately cigar-shaped. Its core exhibits a high degree of spheroidal symmetry and a bright, concentrated luminosity gradient, suggesting an older stellar population. The galaxy displays a color gradient, transitioning from a bluer hue in the outer regions to a yellower/redder tone closer to the nucleus, indicative of variations in stellar population age and metallicity. Evidence of a disk-like structure is not immediately apparent. The overall smooth appearance indicates the likelihood of established morphological stability, showing little signs of recent major mergers or significant tidal disturbances. This galaxy is likely a relatively massive system with suppressed star formation.
