The galaxy presents a generally smooth and elliptical morphology. It appears relatively compact, exhibiting a concentrated central region that gradually diffuses outwards. The color profile suggests a population dominated by older stars, with a yellowish hue at the core transitioning to slightly redder tones in the outer regions. There is a faint hint of greenish color that may indicate some star formation. No prominent spiral arms or significant dust lanes are discernible. Overall, the galaxy exhibits characteristics consistent with an elliptical galaxy, although the low resolution obscures finer details. The galaxy does not obviously show any signs of disturbances or merging events.
