The galaxy presents as a moderately luminous, elongated structure. It displays a generally smooth morphology with a noticeable central bulge. The bulge appears to be a significant component, exhibiting a concentrated distribution of light. There is a subtle color gradient observed, with a yellowish-orange hue dominating the central region, potentially indicating an older stellar population. The outer regions of the galaxy exhibit a faint, bluish tint, which may be indicative of younger stars and ongoing, albeit subdued, star formation. The overall shape appears to be an elliptical form, leaning toward a cigar-like shape. There is no obvious evidence of a recent major merger, nor any signs of tidal tails or significant morphological disturbances.
