This galaxy presents a generally smooth and rounded morphology. The central region exhibits a high concentration of light, appearing as a bright, yellowish core. There is a subtle extension of light surrounding the core, suggesting a possible disk component, although distinct spiral arms are not discernible in this image. The overall color of the galaxy appears relatively red, hinting at an older stellar population. There is minimal evidence of significant dust lanes or active star-forming regions within the visible structure. No prominent features indicating a major merger are apparent. Subtle features suggest the possibility of a minor gravitational disturbance.
