The galaxy presents an overall elongated morphology with a bright, concentrated core. The light distribution appears relatively smooth, indicating a potentially evolved stellar population and a lack of significant ongoing star formation in the central regions. A slight color gradient can be observed, with the core exhibiting a yellower hue compared to the slightly bluer, more diffuse outer regions. The isophotes appear elliptical. The galaxy appears to be undergoing a merger with what appears to be a smaller spiral galaxy nearby to the bottom. The tidal disruption is not very severe, likely indicating that this is an early-stage merger.
