The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its shape is approximately round, showing only a slight deviation from perfect circularity. There is evidence of subtle disturbances in its morphology, possibly indicative of a minor interaction or internal activity. While the majority of the galaxy's light is concentrated in the central region, there is a faint, extended halo surrounding the core. The color profile suggests a mix of stellar populations, with a tendency towards slightly redder hues. This could indicate the presence of older stars and/or dust obscuration within the galaxy. Overall, the galaxy appears to be a relatively quiescent system, though not completely undisturbed.
