The galaxy presents as a roughly elliptical structure, appearing largely featureless and smooth in texture, with minimal evidence of spiral arms or dust lanes. Its color profile suggests a dominance of older stellar populations, exhibiting a reddish-yellow hue. The overall round morphology is indicative of an early-type galaxy, likely an elliptical or lenticular galaxy, with an estimated diameter of about 4.4 kpc. There is no strong visual indication of ongoing major star formation, nor significant tidal disturbances or signs of an active galactic nucleus. While a merger cannot be completely ruled out, there is no substantial morphological evidence to support such an event. The galaxy exhibits high luminosity across all bands, suggesting a sizable stellar mass. The colors indicate the presence of a well-evolved stellar population, with minimal blue light suggesting very low ongoing star formation.