This galaxy presents a moderately bright, somewhat elongated morphology. The central region exhibits a concentrated, yellowish-white luminosity, suggestive of an older stellar population. Extending from this central region is a fainter, bluer component, potentially indicative of ongoing star formation. This blue component appears disturbed or irregular in shape, possibly suggesting an interaction or merger event in its recent history. Overall, the galaxy appears as a system that is somewhere between an elliptical and spiral type, with some evidence of recent or ongoing activity.
