The galaxy presents as a relatively smooth, elliptical structure with an observed color gradient shifting from a yellowish core to a slightly redder halo. The galaxy's morphology is largely featureless, displaying no prominent spiral arms or bar structures. It appears moderately rounded, showing little sign of elongation or asymmetry, potentially indicating a classification along the E3-E5 range on the Hubble sequence. The central region is significantly brighter and more concentrated than the outer regions, suggesting a possible active galactic nucleus or a dense stellar population in the galactic bulge. There is no clear evidence of ongoing major mergers or significant tidal disturbances from the galaxy's overall shape and structure. The color suggests an older stellar population.
