The galaxy presents as an elliptical structure with a noticeable bulge. The central region exhibits a concentrated luminosity, indicating a high stellar density, consistent with an older stellar population. The light profile appears smooth, with a gradual decrease in intensity from the core to the outer regions. The galaxy is tilted relative to our line of sight, with an axial ratio indicating it is somewhat flattened. Faint, extended features are tentatively observed at the edges, but there is no clear spiral arm structure or dust lane obscuration visible in the image. Overall, the galaxy appears to be an early-type galaxy at a redshift of approximately 0.12, suggesting a considerable distance. The color profile transitions from yellowish-white in the bulge, indicating older stars, to a more subtle bluish-white towards the edges, implying younger and hotter stars or more recent star formation activity in the outskirts. There may be evidence of minor disturbances in the galaxy, such as slight asymmetries in the outer halo.
