The galaxy presents a generally elongated, cigar-shaped morphology. It exhibits a smooth light distribution, indicative of a relatively homogenous stellar population. The color gradient displays a concentration of yellowish light towards the central region, transitioning to a slightly bluer hue at the outer edges. This color variation suggests the presence of younger, hotter stars in the galaxy's periphery, possibly resulting from ongoing star formation. No distinct spiral arms or prominent features are discernible within the observed structure, leading to a classification potentially leaning towards an elliptical or lenticular type. The absence of significant morphological disturbances suggests it is not currently undergoing a major merger event.
