The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, with a round shape. The light profile exhibits a strong central bulge, which fades gradually towards the outer regions. There is no apparent disk structure, spiral arms, or bar.

The galaxy displays a color gradient, transitioning from a yellowish-white core to bluish hues in the outer regions. This could suggest a population of older stars concentrated in the core, with younger, bluer stars in the surrounding regions. The smoothness of the galaxy's light distribution and the lack of significant morphological disturbances suggest it has not undergone a major merger recently, though there may be evidence of minor disturbances present. The absence of strong dust lanes further supports the classification of this galaxy being elliptical.
