The galaxy presents as an elliptical or lenticular type, characterized by a largely smooth and concentrated light distribution. There is little to no apparent spiral arm structure, lending to the classification of the galaxy as smooth. The isophotes appear generally rounded with only slight deviations towards a cigar shape. The color profile suggests a more prominent population of older stars, contributing to its yellowish-white hue in the central region. Faint extensions emanate from the core, though they are ill-defined, potentially suggesting a relatively quiescent state without major ongoing starburst activity or recent mergers. There is no obvious dust lane or significant feature suggesting an active galactic nucleus. A slight visual asymmetry may indicate a minor interaction or disturbance.