The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth morphology with a slight elongation. It presents a centrally concentrated luminosity profile, with a core of high surface brightness gradually decreasing outward. The color profile is suggestive of an older stellar population, indicated by the predominantly yellow-red hue. There is a subtle hint of bluer colors at the edge, which may indicate younger, hotter stars, but this needs verification via color analysis. There is no apparent spiral structure or bar, and no indication of recent major merger events. The galaxy exhibits a moderate amount of stellar mass, with signs of ongoing but low levels of star formation.