The galaxy presents as a moderately luminous object exhibiting a smooth, elliptical morphology. The color gradient suggests a relatively evolved stellar population, with a dominant yellowish-orange hue concentrated toward the central regions. There is a lack of distinct spiral arm structures or prominent dust lanes, further supporting the classification of the galaxy as elliptical. Its roundness appears slightly distorted with a cigar shaped fraction, suggesting possible tidal interactions with another galaxy or some ongoing or past perturbation. The overall structure of the galaxy appears relatively undisturbed, with no major signs of merging activity.
