The galaxy exhibits a disk-like morphology, though appearing somewhat rounded in overall shape. Its surface brightness distribution seems relatively smooth, lacking prominent spiral arms or concentrated knots of star formation. A slight elongation is visible, suggesting a possible oblate spheroid shape. The color profile indicates a general homogeneity, with a subtle central concentration of slightly redder hues, indicative of an older stellar population toward the galaxy's core. There are no obvious signs of ongoing major merger activity or significant tidal disturbances.