The galaxy presents a predominantly smooth morphology, with a relatively high degree of central concentration. Its shape appears to be somewhere between round and elongated, with a slight preference for being in between. The color profile suggests an older stellar population dominating the light output, exhibiting a yellowish-red hue. There is a small degree of bluer light present in the outer regions, possibly indicating some ongoing or recent star formation in those areas. No major merger events are apparent in the galaxy's structure; however, the overall shape is slightly asymmetric, possibly indicating a minor disturbance. The galaxy is a relatively massive system with moderate to low level of star formation.
