The galaxy presents as a centrally concentrated object, exhibiting a predominantly smooth morphology. The central region displays a yellowish hue, suggestive of an older stellar population and potentially lower levels of ongoing star formation. There are very faint hints of a slight disk like structure, with faint extensions that may be spiral arms. The galaxy appears to be mostly undisturbed, with no significant signs of tidal features or ongoing major mergers. Its overall roundness suggests that it might be closer to an elliptical or S0 type galaxy, rather than a spiral with well-defined arms, though it may be a smooth spiral galaxy.
