The galaxy presents an elongated morphology, appearing approximately 7 arcseconds in its effective radius. The galaxy's central region displays a bright, relatively smooth luminosity profile. Extending outward, the galaxy exhibits a diffuse structure with faint, irregular features. There are hints of tidal disruption. There appears to be a faint, extended tail of stellar material or gas emanating from the main body, suggesting possible interaction or recent merger activity. Overall, the galaxy appears disturbed, and its asymmetry points towards a dynamic environment.
