The galaxy presents an overall elliptical morphology, appearing elongated with a cigar-shaped profile. It exhibits a relatively smooth structure, with minimal visible signs of distinct spiral arms or significant irregularities. A slight color gradient can be observed; the central region displays a more yellowish or reddish hue, potentially indicating an older stellar population or dust concentration. Progressing outwards, the surrounding regions gradually transition into a bluer tint, suggestive of younger stars or a reduced level of dust obscuration. There is some indication of a minor disturbance, possibly suggestive of a recent interaction with a small companion galaxy. The galaxy is estimated to be of moderate mass with low to moderate star forming potential.
