The galaxy presents an elliptical morphology, appearing highly elongated with a cigar-like shape. Its light profile suggests a smooth distribution of stars, lacking distinct features such as spiral arms or a prominent central bulge. There is a concentration of light towards the center of the galaxy, indicating a higher stellar density in the core. The color gradient transitions from a yellowish-white central region to a redder hue at the edges, potentially indicating a higher population of older stars in the outer regions or dust obscuration. No significant signs of tidal disturbances or interactions with other galaxies are evident in this image, which points to it being a relatively isolated system with little to no evidence of recent mergers or ongoing starburst activity.
