The galaxy presents as a smooth, somewhat elliptical structure with a high degree of central concentration. The color profile suggests an older stellar population, exhibiting a redder hue compared to galaxies with ongoing star formation. There appears to be minimal evidence of spiral arm structures or significant dust lanes. The galaxy's overall appearance indicates a morphology that is likely classified as an early-type galaxy, possibly an elliptical or lenticular. There may be some signs of minor disturbances to the morphology, suggesting a past or ongoing interaction with another galaxy, though not a complete merger. The roundness suggests a lack of a defined disk, supporting the elliptical classification.
