The galaxy presents a primarily smooth morphology with some notable features. The central region exhibits a bright, concentrated core, suggestive of an active galactic nucleus or a dense stellar population. A disk-like structure is visible, though it is somewhat irregular and not sharply defined. There are indications of minor disturbances or asymmetries within the disk, possibly due to past interactions or internal dynamics. No clear spiral arms are discernible. A slight color gradient can be observed, with the central regions appearing bluer than the outer parts of the disk. This difference might indicate varying stellar populations, with younger, hotter stars dominating the central regions. There might be a very faint plume. Overall, the galaxy appears to be relatively isolated, with no apparent signs of ongoing major merging activity.
