The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing moderately rounded in shape. A slight disturbance in the symmetry is suggested by a subtle extension or asymmetry on the galaxy's periphery, which could be the result of a minor interaction or internal dynamics. The galaxy's color profile suggests the presence of moderate star formation activity. It exhibits a blueish tint towards the central region, likely indicating the presence of younger, hotter stars, transitioning to redder hues in the outer regions, possibly indicative of an older stellar population. There is no obvious barred structure or prominent spiral arm features visible in this image. Overall, the galaxy appears as a relatively evolved system, with no major ongoing merger events.
