The galaxy presents as an elliptical morphology, with a high degree of central concentration and a relatively smooth overall appearance. The light distribution exhibits a noticeable elongation, appearing somewhat cigar-shaped. The core is a bright, luminous yellowish-white, indicative of an older stellar population. The outer regions exhibit a color gradient, transitioning to a faint reddish hue, potentially suggesting a declining rate of star formation. There is no apparent dust lane or distinct spiral arm structure. A slight asymmetry might be present, but this would require further investigation.
