The galaxy presents an overall elliptical morphology, appearing cigar-shaped. A smooth light distribution indicates it is most likely an early-type galaxy. There is a distinct central bulge that appears a slightly warmer color, possibly indicative of an older stellar population or dust absorption. Fainter, bluer light extends along the major axis, suggesting the possibility of some star formation activity, or a disk component, despite the overall smooth appearance. There is no evidence of tidal features or significant morphological disturbance, suggesting that it has not undergone a major merger recently. Based on the overall color, it seems to be a massive system with a relatively low star formation rate.
