The galaxy exhibits a morphology suggestive of a late-stage merger. Its light profile appears dominated by a smooth, elliptical component with an overall slightly elongated shape. There is a prominent central bulge exhibiting a yellowish-orange color, indicating a population of older stars and likely dust obscuration. Dispersed areas of blue-green hint towards more recent or ongoing star formation. Asymmetrical features are noted, which is consistent with a gravitational interaction. There is a notable tidal tail or similar disruptive structure extending from the main body, indicating the presence of past tidal interactions.
