The galaxy presents a generally smooth and elliptical morphology, with a centrally concentrated luminosity profile. There is a subtle, extended halo surrounding the brighter core, which suggests a more diffuse distribution of stars at larger radii. The color gradient transitions from a redder hue in the central regions to slightly bluer tones in the outer parts of the halo. No distinct spiral arms or prominent dust lanes are discernible, leading to a classification of the galaxy as likely an elliptical or S0 type. There is no evidence of active galactic nuclei features or morphological indications of recent major merger events. Subtle asymmetries may indicate minor tidal interactions or internal dynamics.
