The galaxy presents as a roughly elliptical, yet somewhat irregular, structure. The central region exhibits a yellowish hue, indicating a population of older stars. There is a faint blue tinge towards the edges, possibly suggestive of some ongoing, albeit limited, star formation in the outer regions. The galaxy appears largely smooth in texture, with no distinct spiral arms or prominent dust lanes visible. There is also an absence of any clear signs of a recent major merger or significant tidal disturbances. Overall, the galaxy seems to be a relatively evolved system, with a dominant, aging stellar population.
