The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of concentration, characterized by a bright, yellowish-orange hue, suggesting an older stellar population and potentially a lower rate of on-going star formation. The overall shape is elongated, appearing neither perfectly spherical nor highly flattened. There is no clear evidence of prominent spiral arms, dust lanes, or significant tidal disturbances indicative of recent major merger events. Subtle color variations are observed in the outer regions, with hints of bluer light, possibly representing a younger stellar population. Faint irregularities are present in the outer regions of the galaxy, suggesting a possibility of some minor mergers, but the galaxy is generally undisturbed.
