The galaxy appears as a single, relatively smooth object with a concentrated light profile. Its shape is generally round, with no obvious distortions or tidal features indicative of recent major mergers. There may be a slight elongation, but it is subtle. The color distribution suggests a dominant population of older stars with a redder hue. There are hints of possible minor disturbances, but they do not dominate the galaxy's overall morphology. Its estimated size is of an intermediate dimension, neither exceptionally large nor particularly compact. Its star formation rate appears relatively low, classifying it as a quiescent or passively evolving system.