The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a pronounced radial gradient in luminosity, peaking sharply towards the center. The color profile suggests a population of older stars dominating the central region. There is a subtle decrease in redness with increasing radius, hinting at a slightly younger stellar population in the outer regions. There is no apparent spiral structure or significant dust lane obscuration. The overall impression is that of a relatively undisturbed galaxy with minimal ongoing star formation. Faint asymmetries in the outermost regions may indicate minor tidal interactions.
