The galaxy presents an elliptical morphology, appearing elongated with a high degree of axial ratio. There is evidence of a relatively smooth light distribution within the galaxy's body, indicative of an older stellar population and minimal recent star formation. The color gradient suggests a possible presence of a redder core, potentially due to dust or older stars concentrated towards the center. Faint blue tinges may be present, but these are minimal, likely indicative of a suppressed, yet extant, star formation activity. No distinct spiral arm features are readily apparent. Overall the galaxy appears to have experienced quiescence, and there is no significant sign of a ongoing major merger event, but subtle tidal disruption of this system cannot be ruled out.
