The galaxy presents as a somewhat amorphous, elliptical structure with a high degree of central concentration. Its color profile suggests a population of older stars, emitting primarily in the redder bands of the spectrum. The overall morphology appears smooth with no evidence of distinct spiral arms or a prominent disk. There is a slight elongation visible, but the object is generally rounded. The galaxy exhibits no obvious signs of major mergers or tidal disturbances. The light distribution is relatively even, with the majority of luminous material concentrated towards the core, indicating a possible evolved stellar population. There is evidence of ongoing, but perhaps relatively subdued, star formation activity. 
