The galaxy presents as an elliptical or lenticular structure with a generally smooth, diffuse appearance. Its central region is brighter and exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer light is distributed irregularly throughout the disk, potentially indicating regions of more recent, though likely subdued, star formation. The overall morphology suggests a relatively evolved system, with minimal evidence of a spiral structure or actively merging components. The galaxy appears elongated, indicating a possible cigar shape. There may be another small galaxy near it.