The galaxy presents as an elongated, spindle-shaped structure, suggesting it is likely an elliptical galaxy viewed nearly edge-on. The luminosity profile appears smooth and centrally concentrated, with a gradual decrease in brightness towards the outer edges. There is a lack of distinct spiral arm features or prominent dust lanes, which are characteristic of spiral galaxies. The galaxy exhibits a predominantly blue hue, implying that it may contain a substantial population of young, hot stars. The morphology suggests a low rate of recent mergers or major disturbances and also indicates that this galaxy is rounder than average. Overall, this galaxy's morphology hints at a moderately massive system with a relatively low star formation rate.
