The galaxy presents as a generally smooth, elliptical or lenticular object with a high degree of central concentration. It exhibits a bright, yellowish-orange core, potentially indicative of an older stellar population dominated by red giant stars and a lower rate of ongoing star formation. The outer regions of the galaxy appear fainter with a subtle disk-like morphology, hinting at a possible transition in stellar populations or past merger event. The galaxy is elongated, appearing cigar-shaped, with no significant signs of tidal disturbances or active galactic nuclei in this imaging. The observed color gradients suggest a radial change in stellar population, with the core likely more metal-rich and the outer regions perhaps containing a younger, bluer population, despite the overall smoothness. The overall appearance implies that the galaxy is relatively isolated. 
