This galaxy presents as a relatively smooth, elliptical morphology with an apparent lack of distinct spiral arms. The central bulge exhibits a concentrated, yellowish hue, suggestive of an older stellar population. The outer regions display a bluer tint, possibly indicating some ongoing, though not extensive, star formation. The galaxy appears elongated, rather than perfectly spherical. There is a potential, small tidal disturbance on one side, which could imply a past or ongoing minor interaction with another galaxy, however, there does not appear to be any major interaction at the current time. Overall, it appears to be an intermediate mass galaxy with a moderate amount of star formation.
