The galaxy appears as a slightly elongated, elliptical object with a smooth, concentrated light profile. The core is a bright, yellowish-white color suggesting a population of older stars. There is a faint, bluish halo surrounding the core, possibly indicating a lower level of ongoing star formation or a population of younger stars in the outer regions. The overall structure lacks distinct features such as spiral arms or a bar, lending further support to an elliptical classification. There is no clear evidence of any major mergers or significant tidal disturbances affecting the galaxy's morphology. The galaxy seems relatively isolated and undisturbed.