The galaxy presents a generally smooth morphology, suggesting an elliptical or lenticular type. The light distribution appears centrally concentrated, with a gradual decrease in brightness towards the outer regions. The overall shape is moderately elliptical, appearing somewhat elongated but not highly cigar-shaped. There is a subtle hint of a possible minor disturbance in the galaxy's structure; this may be due to either a weak tidal interaction or the result of an internal feature. No clear evidence of a major ongoing merger is apparent. The galaxy appears to have a blue-green hue. The galaxy's color could point to ongoing star formation, though a redder, more elliptical galaxy is likely.
