This galaxy appears to be a relatively smooth, single object with minimal visible substructure. Its overall shape is somewhat round and compact, displaying a centrally concentrated brightness profile that fades gradually towards its outer regions. The galaxy exhibits a yellowish-white hue in the central region, which could potentially indicate an older stellar population with lower levels of ongoing star formation. There is a hint of bluer emission at the edges of the galaxy, which could indicate a small amount of star formation is present.

The lack of a distinct spiral arm structure or a prominent bulge suggests this may be a relatively early-type galaxy, although some subtle disturbances may be present. The galaxy's luminosity appears to be relatively high, indicating it is reasonably massive. There does not appear to be evidence of a major ongoing merger or significant tidal interactions.
