The galaxy appears to be a relatively smooth, round object with a concentrated central bulge. Its color is primarily blue-white, which suggests a population of younger, hotter stars. There is little evidence of spiral arms or significant dust lanes. The galaxy does not exhibit any obvious signs of ongoing major mergers or tidal disturbances. Given its morphology, it's likely an early-type galaxy, possibly an elliptical or lenticular type. The apparent lack of distinct features may also indicate it is a more distant object, and finer details are not easily resolvable at this scale.
