The galaxy presents as a roughly elliptical object, with an estimated effective radius of approximately 4 kiloparsecs. Its overall color appears yellowish-white, suggesting a relatively older stellar population. The morphology indicates a predominantly smooth structure, with a noticeable concentration of light towards the central region. There is evidence of an ongoing or recent interaction or merger event. A distinct secondary concentration of light is observed, slightly offset from the main body, possibly indicating a smaller galaxy being tidally disrupted or a region of intense star formation triggered by the interaction. The tidal feature exhibits a redder color, which could potentially indicate a difference in stellar population between the main galaxy and this interaction feature. There are no clear spiral arm features evident, and it is not an obvious disk galaxy.
