The galaxy presents as a centrally concentrated, luminous object with a generally smooth morphology. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. There is a subtle decrease in intensity moving outward from the core, but there is not a prominent disk-like structure nor any obvious spiral arms. Faint extensions or irregularities can be seen around the core. These could be due to tidal interactions, minor disturbances, or some slight star formation. Overall, the galaxy appears round.
