The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. The galaxy has a slightly elongated shape, suggesting a moderate degree of ellipticity. The color profile indicates a predominantly older stellar population, emitting light in the redder part of the spectrum. There is no clear evidence of spiral arms or a prominent disk structure. The lack of dust lanes also supports this classification. The core region presents a higher surface brightness, gradually diminishing towards the outer edges. There are no obvious signs of active galactic nuclei activity or ongoing mergers. The overall appearance suggests a galaxy that has largely exhausted its gas reserves and experienced a decline in star formation activity.
