The galaxy appears as an elongated, cigar-shaped structure, indicative of an elliptical morphology. The central region exhibits a bright, concentrated luminosity, with a primarily yellow hue. Fainter, reddish extensions are observed at the periphery, potentially signifying older stellar populations or dust lanes. There is no clear evidence of spiral arms or active star formation regions. Overall, the galaxy presents a relatively smooth texture, suggesting a lack of major disturbances or ongoing merging events. The overall color is redder than typical spiral galaxies, with g-r color of 1.33 and r-z color of 0.87, suggesting it contains older stars.
