The galaxy presents a morphology dominated by a smooth, centrally concentrated light distribution. It appears ellipsoidal in shape, with a moderate ellipticity. The color profile exhibits a generally blue hue in the central region, gradually transitioning to redder tones towards the outer edges. This color gradient suggests a potential variation in stellar population, with younger, bluer stars concentrated towards the core and older, redder stars populating the outskirts. There is minimal visual evidence of prominent spiral arms or distinct star-forming regions. Subtle irregularities or minor disturbances are possibly present within the disk, but not prominently. There does not appear to be any evidence of recent major merger activity.
