The galaxy presents as a slightly elongated, lenticular-like object. Its central bulge appears relatively bright and well-defined, exhibiting a smooth, symmetrical profile. The surrounding disk, while present, lacks distinct spiral arm structures. Its colors are consistent with an older stellar population, predominantly exhibiting light in the redder wavelengths. There is no evidence of significant dust lanes or active star formation regions visible in this image. Overall, it appears to be a relatively evolved galaxy, likely transitioning towards an elliptical morphology. There may be some minor disturbances present, possibly indicating a past or ongoing interaction with another galaxy.
