The galaxy presents a largely smooth morphology, with a high degree of central concentration. The light distribution appears nearly elliptical, transitioning from a bright, compact core to a fainter, diffuse outer envelope. The color profile suggests a subtle radial gradient, with the central regions exhibiting a bluer hue compared to the redder periphery. There is little evidence of prominent spiral arms or distinct structural features. The overall appearance is consistent with that of an early-type galaxy, potentially an elliptical or lenticular galaxy viewed at a considerable distance. Subtle distortions are apparent, possibly indicative of minor tidal interactions. Star formation is subdued, but is likely more pronounced in the central region.
