The galaxy presents as a somewhat elliptical, moderately luminous object. Its central region exhibits a concentrated, bright yellow-white hue, suggesting a high density of older stellar populations. The light appears to gradually diminish and redden toward the outer regions of the galaxy, indicating a potential decrease in stellar density and/or a change in stellar population composition. There is no readily discernible spiral structure or prominent dust lanes. The galaxy's overall morphology appears smooth and relatively undisturbed. Subtle asymmetry in the outer regions could possibly suggest a minor interaction or tidal disturbance, though more data would be needed to support this.
