The galaxy presents as a centrally concentrated object with a mostly smooth morphology. There appears to be a gradual fading of intensity from the core outwards, suggesting a lack of distinct spiral arm structures or a well-defined disk. The general shape is somewhat elliptical, but approaching round, with the color profile trending redder towards the center. There is no obvious evidence of ongoing major merger activity or significant tidal disturbances, though faint and subtle irregularities in the outer regions cannot be entirely ruled out. The overall appearance indicates a galaxy that is likely dominated by an older stellar population, exhibiting a low rate of star formation.
