The galaxy presents as a centrally concentrated object, characterized by a smooth morphology. The dominant light emission is observed in the yellow-red portion of the spectrum, which is indicative of an older stellar population. There appears to be a slight, extended halo surrounding the central region. The galaxy lacks any obvious spiral arm structure or significant dust lanes. The shape is largely spherical, with no discernible elongation. There is no evidence of any on-going merger events or major tidal disturbances. The galaxy exhibits a relatively high degree of smoothness, suggesting it is likely an elliptical galaxy. The lack of blue light and presence of redder colors also supports this classification. Overall, the visual assessment indicates a relatively quiescent galaxy with a primarily evolved stellar population.
