The galaxy exhibits a generally smooth morphology. It presents an elongated, cigar-shaped appearance. A subtle feature is potentially an indication of a minor disturbance, but does not immediately suggest a major merger event. The galaxy displays a color gradient, with a central region that appears yellower, possibly indicating a higher concentration of older stellar populations, and outer regions that are bluer, potentially indicative of ongoing star formation. Overall, the galaxy appears to be a relatively massive system.
