The galaxy appears to be a relatively smooth object, likely an elliptical or lenticular type. Its shape is elongated, exhibiting a cigar-like morphology. There is a bright central bulge that fades gradually into the outer regions. The color profile suggests a dominant population of older stars, particularly in the bulge, with a yellowish or golden hue indicating a lack of recent star formation. There might be some slight disturbances or asymmetries present, but it generally appears as a single, relatively undisturbed object. The lack of prominent spiral arms or distinct features points toward a classification of a galaxy with a more spheroid-dominated structure.
