The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. It appears to have a notable central bulge region that is brighter and more densely packed than the surrounding regions. There's little evidence of strong spiral arm structure or prominent dust lanes in the image. The overall color profile suggests a population of older stars, with a tendency toward redder hues, though the core shows some evidence of bluer light. The galaxy exhibits a degree of interaction or minor disturbance.
