The galaxy presents a relatively smooth, elliptical morphology. The core exhibits a concentrated luminosity profile, appearing yellowish-white in color, suggesting an older stellar population with limited ongoing star formation. A fainter, bluish haze extends from the primary body, particularly on one side, potentially indicative of a tidal tail or a region of more recent star formation. There are no prominent spiral arm structures discernible. The overall shape is somewhere between round and elongated, with no indication of significant disturbances that would strongly indicate a major merger event, although a past or ongoing minor interaction cannot be ruled out. The galaxy appears to be a substantial system, based on its overall luminosity.
