The galaxy presents as a compact, relatively smooth object with a concentrated central region. It exhibits a generally elliptical morphology, appearing more rounded than elongated. A slight color gradient is observable, with the central region appearing distinctly bluer compared to the outer regions which possess a redder hue. This may indicate ongoing star formation within the core and/or a difference in stellar populations between the nucleus and the outer parts of the galaxy. There is no clear evidence of spiral arm structure or significant tidal disturbances, suggesting the galaxy is relatively undisturbed. However, subtle irregularities in the light distribution may hint at minor interactions or internal dynamic processes.
