This galaxy appears to be an elliptical galaxy. It presents with a generally smooth and rounded morphology. The color profile indicates a population of older stars, skewed towards the redder end of the spectrum. There is no strong evidence of spiral arms or a prominent disk structure. The galaxy lacks significant dust lanes or patches of ongoing star formation, supporting the classification as an elliptical galaxy with a relatively low star formation rate. There may be a very slight tidal feature that could indicate a minor disturbance event. The galaxy has high central concentration.
