The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration. The light distribution indicates it is somewhat elongated, appearing cigar-shaped along its major axis. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. There is a lack of prominent spiral arm structure or significant dust lanes visible. Faint, diffuse light extends outwards from the central region, fading gradually into the background sky. There are subtle indications of disturbance in the outer regions of the galaxy. Based on the image, the galaxy does not appear to be undergoing a major merger, nor does it have any prominent features of merging activity. The light distribution is generally consistent with an elliptical galaxy, with possibly some indications of a disk galaxy.
