The galaxy presents as a somewhat elongated structure. The central region exhibits a concentrated, smooth appearance, with a yellowish hue suggestive of an older stellar population. Fainter, diffuse extensions are visible emanating from the central region, particularly towards the upper portion of the galaxy. These extensions show subtle variations in color, with hints of bluer regions possibly indicating areas of more recent star formation, though at a low rate. The overall morphology appears relatively undisturbed, without strong evidence of a recent major merger. However, there might be minor irregularities suggesting past or ongoing interactions.
