The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. Its shape is elongated, with a high degree of ellipticity, indicating a cigar-like structure. There is no evidence of spiral arms or a prominent galactic disk. The central region appears to be dominated by older stars, emitting light in the redder part of the spectrum. A faint gradient suggests some ongoing, though likely subdued, star formation activity in the outer regions, indicated by subtle blue-green hues. No significant disturbances or merging events are apparent, suggesting a relatively quiescent evolutionary state. The galaxy's light output suggests a moderately luminous object, indicative of a substantial stellar mass.
