This galaxy presents a somewhat elliptical morphology, appearing nearly edge-on from our vantage point. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population. The outer regions are less defined, showing a more diffuse distribution of light. There are hints of spiral arm structures, though these are not clearly resolved in the image. The color gradient suggests a variation in stellar populations, with bluer hues potentially indicating ongoing star formation and redder hues potentially indicating older stellar populations. There are no signs of a major merger, but a slight disturbance cannot be ruled out.
