The galaxy presents as a relatively smooth, elliptical morphology, with a centrally concentrated luminosity profile. The core exhibits a yellow-orange hue, suggesting an older stellar population. The isophotes are generally regular, indicating a lack of significant tidal disturbances or recent major mergers. A subtle flattening can be observed, indicating some degree of ellipticity. Faint, diffuse light extends outwards from the central region, gradually fading into the background sky. There is no indication of prominent spiral arms or substantial dust lanes. The overall appearance is consistent with an early-type galaxy at a moderate redshift, potentially exhibiting low levels of ongoing star formation.
