The galaxy appears as a relatively small, elongated object. Its color profile suggests a mixture of stellar populations, with a dominant blue-green hue in the central region that could indicate ongoing star formation. The galaxy exhibits a smooth morphology, with a subtle central condensation. The overall shape is reminiscent of a flattened spheroid, significantly longer than it is wide, displaying a cigar-like appearance. There is no obvious evidence of major mergers or strong tidal features, though there may be some minor disturbances in the outer regions. The smoothness and color profile suggest a possible transition between a spiral and elliptical galaxy, and low levels of star formation.
