The galaxy presents a generally elliptical morphology, exhibiting a high degree of central concentration. Its color profile suggests a primarily older stellar population, with a dominant yellowish-red hue emanating from the core. Fainter, diffuse greenish-yellow emission extends outwards from the central region, which may indicate regions of ongoing, albeit subdued, star formation activity or potentially the presence of ionized gas. The lack of clear spiral arm structures or distinct morphological features implies a relatively smooth stellar distribution. There is little evidence of significant tidal disturbances or mergers with other galaxies in its immediate environment, with the galaxy's overall appearance suggesting relative quiescence. The outer regions appear to be fading into a hazy cloud, indicative of a large, sparse halo of older stars. 
