The galaxy appears to be a relatively smooth, round object with a concentrated central bulge. It exhibits a yellowish hue, suggesting a population of older stars and potentially a lower rate of ongoing star formation. There is little evidence of spiral arm structure or significant dust lanes; its features are rather homogenous and somewhat spheroidal. There might be a very faint hint of a surrounding halo or extended stellar envelope, but that is difficult to say definitively. Based on the features displayed, it's likely that the galaxy is a relatively massive system. It does not appear to be undergoing any major merging activity, though minor tidal disturbances cannot be ruled out from this image alone.
