The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. The central region exhibits a pronounced concentration of light, suggesting a well-defined nucleus or bulge. The color gradient indicates a relatively older stellar population, with a yellowish to reddish hue dominating. There is a faint disk structure with some evidence of possible spiral arm fragments. The image suggests limited ongoing star formation within this galaxy, although some activity may be present. There does not appear to be significant dust lanes or strong tidal features associated with this object, implying it is likely not undergoing a major merger.
