The observed galaxy presents as a centrally concentrated light source with a relatively smooth appearance. The core region exhibits a bright, nearly uniform luminosity, transitioning into a diffuse outer halo. The halo displays an irregular shape, with slight extensions evident. There is marginal distortion, indicating that it may be interacting with another galaxy. The galaxy's color profile suggests a possible mixture of stellar populations, with a bluer hue emanating from the core possibly indicative of a younger stellar population. The outer regions transition to a redder color, suggesting older stars. Overall, this galaxy exhibits a primarily elliptical morphology with slight disturbances to its overall shape.
