The galaxy presents as a relatively compact, elliptical structure with a smooth, diffuse light distribution. The central region exhibits a concentration of yellow light, suggesting an older stellar population dominating the core. There is a subtle gradient in color towards the outer edges of the galaxy, transitioning from yellow to a slightly redder hue. This may indicate the presence of a population of evolved, redder stars or dust obscuration in the outer regions. There is no evidence of prominent spiral arms, distinct star-forming regions, or significant tidal disturbances. The overall morphology suggests a mature galaxy that is undergoing limited current star formation.
