The galaxy presents a somewhat smooth, slightly elongated morphology, trending towards a cigar shape. It appears primarily smooth with a likely lack of prominent spiral arm structures. The galaxy exhibits a color gradient, with a central, concentrated region that appears more yellow-orange, suggesting an older stellar population. Fainter, bluer patches are distributed around the central region of the galaxy, indicating areas of more recent star formation, albeit at a relatively low rate. There is no indication of ongoing major merger activity, although a minor disturbance within the structure cannot be entirely ruled out. The galaxy is relatively compact.
