The galaxy presents as a relatively smooth, elliptical structure. The light distribution appears centrally concentrated with a yellowish hue, suggesting a population of older stars. There is little evidence of prominent spiral arms or active star formation regions within the visible light spectrum. The galaxy is elongated, but not significantly cigar-shaped. There are no obvious signs of major mergers or significant tidal disturbances. Overall, the galaxy exhibits characteristics consistent with a passively evolving, early-type galaxy.
