The galaxy presents a generally smooth, rounded morphology. Its light profile appears centrally concentrated with a bright core that gradually fades towards the outer regions. There is a subtle colour gradient visible, with the central region displaying a yellowish hue, possibly indicating an older stellar population, while the outer regions appear slightly bluer, which may signify the presence of younger stars, though not definitively, given the resolution. No distinct spiral arm structures or prominent dust lanes are discernible. There is no clear evidence of any ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy.
