This galaxy appears to be relatively compact, displaying a bright, somewhat concentrated central region. The light profile suggests a mixture of colors, with a dominant yellowish-white core indicating a substantial population of older stars. There is evidence of a fainter, more diffuse, blue component within the central region, possibly indicative of recent star formation. A reddish area on the right suggests potential dust obscuration or the presence of a population of redder, older stars in that region. The morphology is not clearly defined as purely elliptical or spiral. Instead, it exhibits features of both with some disturbed structure and potentially indicative of a minor interaction or merger event, though a significant portion of the image data is comprised of artifact interference. This observed structure suggests a dynamic and potentially complex formation history.
