The galaxy presents an overall smooth morphology, appearing as a single, relatively featureless object. It exhibits an elongated shape, resembling that of a cigar, rather than a perfect sphere or disk. The color distribution reveals a central concentration of light with a reddish hue, which gradually transitions to a more greenish color toward the outer regions. This color gradient could indicate differing stellar populations or dust distributions within the galaxy, with older stars or a higher dust concentration in the center. Faint disturbances or signs of tidal interactions may be present, suggesting a possible minor past merger or interaction with another galaxy. However, no significant disruptions to the overall smooth structure are observed.
