The galaxy presents as a somewhat irregular structure, appearing perturbed or possibly undergoing a merger event. The central region exhibits a relatively smooth, concentrated light distribution, possibly indicative of an older stellar population.  A distinct, elongated feature extends from the central region, suggesting a tidal tail or stream of stars and gas. This feature displays a bluer color, potentially reflecting ongoing or recent star formation activity.  The overall morphology deviates from a simple elliptical or spiral classification, hinting at gravitational interactions influencing its current shape.  A small, reddish object is closely positioned near the top right of the central region and appears part of the galaxy's structure or a localized region of dust obscuration.
