The galaxy presents an overall smooth morphology, with a concentrated central bulge exhibiting a reddish hue. This likely indicates an older stellar population dominating the core. A fainter, more diffuse disk surrounds the bulge. The disk shows hints of bluer light indicative of ongoing star formation, although it appears relatively quiescent. The galaxy appears to be an intermediate spiral/elliptical galaxy, possibly exhibiting characteristics of both types, such as a disk and a central bulge. There are indications of minor disturbances in the morphology, possibly suggestive of weak tidal interactions or a minor merger event in its past. It has a relatively small angular size and a distance corresponding to a redshift of approximately 0.24, suggesting it is a luminous and massive system despite its moderate star formation rate. 
