The galaxy presents an overall smooth, elliptical morphology. Its color profile appears reddish-gold, suggesting an older stellar population. The galaxy exhibits a centrally concentrated luminosity profile, with brightness decreasing gradually outward. The galaxy's shape deviates slightly from perfectly round, with a hint of elongation. The lack of distinct spiral arms or prominent dust lanes supports a classification favoring elliptical or lenticular types. There is no visible evidence of ongoing major merger activity or significant tidal disturbances affecting the main galactic structure. 
