The galaxy presents a generally smooth appearance, with an elongated, cigar-like shape. There is a brighter, more concentrated central region. The color profile suggests a relatively older stellar population dominating the central bulge, exhibiting a yellow-orange hue. Fainter, bluer regions are observed extending outwards from the central bulge, indicative of ongoing star formation within what appears to be a disk-like component. There is some minor evidence of disturbances in the disk, hinting at possible past interactions or internal dynamic activity. Overall, the galaxy shows characteristics of a system transitioning between a spiral and elliptical morphology.
