The galaxy presents a somewhat amorphous morphology, appearing neither purely elliptical nor a well-defined spiral. There is a central concentration of light that suggests the presence of a core or bulge component. The color profile indicates a mixture of stellar populations. The central region is slightly redder, potentially indicating older, cooler stars or dust obscuration. The outer regions exhibit a bluer hue, which may indicate ongoing or recent star formation activity with younger, hotter stars.

Evidence of disturbances in the galaxy's structure is apparent. A faint tidal feature to the upper left of the galaxy is visible. The galaxy's shape deviates from a perfect ellipse or disk. The overall appearance suggests a galaxy that has potentially undergone a minor interaction or merger event in its recent past. Star formation is actively occurring within the galaxy, with the outer regions possibly hosting some of the star forming regions.
