The galaxy presents a relatively smooth and elliptical morphology. The central region exhibits a high concentration of luminosity, appearing nearly spherical. Progressing outwards, the luminosity gradually decreases without any distinct spiral arm structures or prominent features, such as dust lanes or star-forming regions, visually apparent. The color profile suggests a dominant older stellar population, with a moderate red color in the central region shifting towards a bluer periphery. There is no strong evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy, although a slight asymmetry cannot be entirely ruled out due to limited resolution.
