The galaxy presents as a relatively compact, luminous object. Its morphology is dominated by a smooth, centrally concentrated light distribution. There is minimal evidence of spiral arm structure or prominent dust lanes. The overall color appears slightly redder, suggesting a population of older stars and possibly a lower rate of recent star formation, though it is not completely devoid of blue light. No obvious signs of tidal interactions or ongoing mergers are detected in this image. The light profile suggests that this galaxy is more likely an elliptical or lenticular galaxy.