The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a generally round morphology, with a slight suggestion of an oblate spheroid shape, though the image resolution limits definitive classification. The galaxy has an overall yellowish-orange color, suggesting an older stellar population with lower levels of recent star formation. The light distribution is concentrated toward the center, with a gradual fading towards the outer regions. There is some indication of possible tidal disturbances or interactions, though the dominant feature is its generally smooth and centralized appearance. It could be undergoing a merger, but more data would need to be gathered to confirm that hypothesis.
