The galaxy presents an elongated, somewhat cigar-shaped morphology. It displays a smooth overall appearance, indicating a relatively evolved system. There is a subtle color gradient visible, with a central region appearing more yellow, potentially indicating an older stellar population, and outer regions displaying a bluer hue, possibly indicative of ongoing star formation. No distinct spiral arms or bar structures are readily apparent. There is a suggestion of some minor internal disturbances or irregularities, but these do not dominate the overall structure. The galaxy appears to be relatively isolated with no obvious signs of a major merger event.
