The galaxy exhibits a dominant, centrally concentrated bulge, characterized by a smooth, yellowish-orange hue suggestive of an older stellar population. The overall shape is slightly elongated but mostly rounded with no defined spiral arm structure immediately apparent. There is evidence of a possible minor disturbance or interaction, as indicated by a faint, somewhat detached, secondary concentration of light and color to one side. The main galaxy does not exhibit a strong blue color gradient, indicating low levels of recent star formation. The galaxy's overall color suggests a relatively passive or quiescent state.
