The galaxy presents as an elliptical morphology, appearing largely smooth with a concentrated central bulge. It is elongated in shape, exhibiting a cigar-like form. No distinct spiral arms or bar structures are discernible. The galaxy displays a color gradient, with the central region exhibiting a yellowish hue, possibly indicative of an older stellar population. The outer regions appear somewhat bluer, hinting at the presence of younger stars or ongoing star formation, albeit at a moderate level. There is slight asymmetry, possibly suggestive of a minor gravitational disturbance or interaction with another galaxy, although no clear merger is evident. Overall, the galaxy appears to be a moderately massive system with an active, yet not exceptionally vigorous, star-forming rate.
