The galaxy presents as an elongated, cigar-shaped object. Its light profile suggests a relatively smooth distribution, with a brighter central region and a gradual decrease in luminosity outwards, especially along the major axis. There appears to be a subtle indication of a disk-like structure viewed edge-on. Based on the color indices, the galaxy appears to have a generally blue hue, potentially indicating ongoing star formation, although further spectroscopic analysis would be required to confirm the age and composition of the stellar populations. No significant dust lanes or other distinct features are immediately apparent in the image, but some minor disturbances may be present. Overall, the galaxy appears to be a relatively undisturbed system without strong evidence of a major merger event in its recent history.
