The galaxy appears as a single, relatively smooth object, with a concentrated central region. Its shape is generally round. The color profile suggests a dominant population of older stars, with the central region appearing more yellow-white. There is no discernible spiral structure or prominent dust lanes evident in this image. There is no strong evidence of active star formation regions or HII regions. I observe no indications of tidal tails or distorted features typically associated with recent or ongoing major mergers. There may be minor irregularity to the outer edges of the galaxy.
