The galaxy presents a centrally concentrated morphology, suggestive of an elliptical or lenticular classification. The luminosity appears to be dominated by an older stellar population, inferred from the reddish-yellow hue of the galaxy's core. This color profile indicates a lower rate of recent star formation, consistent with a more evolved system. The isophotes exhibit a generally smooth appearance, showing only a mild deviation from perfect ellipticity. Faint, diffuse extensions of the galaxy's light are observed peripherally, indicating a potential stellar halo extending beyond the main body. There is a suggestion of minor disturbances in the outer regions of the galaxy, possibly due to a past interaction or accretion event. The color gradient transitions gradually from the reddish center to a slightly bluer, albeit still subdued, halo.
