The galaxy presents as a lenticular, cigar-shaped structure with a smooth overall appearance. The central region exhibits a concentrated, bright, yellowish hue, suggesting a significant population of older stars. This central bulge appears elongated along the major axis of the galaxy. Fainter, bluer light extends from the core, tapering towards the edges. These less intense colors are most likely from younger stars. There is minimal evidence of defined spiral arms or dust lanes within the galaxy's disk. No significant tidal features or signs of recent major merger activity are immediately apparent, indicating relative isolation.
