The galaxy presents a largely smooth, elliptical morphology with a highly concentrated central bulge. Its overall shape is generally rounded, displaying minimal deviation from circular symmetry. The light profile appears to gradually fade from the bright core outward, suggesting a lack of distinct spiral arm structures or prominent star-forming regions. The color of the central bulge appears slightly redder compared to the outer regions, which may indicate an older stellar population and reduced star formation activity in the galaxy's core. There are no signs of ongoing major mergers or significant tidal disturbances that could disrupt the galaxy's overall structure. Minor disturbances may be visible in the faint outer regions.
