The galaxy presents as an elliptical morphology, elongated in shape with a high degree of smoothness. The core region appears bright and concentrated, exhibiting a yellowish-white hue suggesting an older stellar population.  Moving outwards from the core, the light gradually fades, with a subtle transition in color towards the edges of the galaxy, where a faint bluish tinge can be observed. This may indicate the presence of some younger, hotter stars in the outer regions, although the overall color profile indicates a lack of significant ongoing star formation. The galaxy does not exhibit any prominent spiral arms or dust lanes, consistent with an elliptical classification. There is no evidence of any major merger events or significant tidal disturbances. The galaxy presents a fairly smooth, regular appearance overall.
