The galaxy presents as a luminous, centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a high degree of radial symmetry, with light intensity decreasing gradually from the core outwards. The galaxy's color appears generally red, with no distinguishable spiral arm structures or prominent dust lanes. The overall smoothness suggests a lack of significant ongoing star formation, and a dominant population of older stars. The galaxy seems to be relatively isolated with no obvious signs of interaction with other galaxies. There is a smaller, less luminous object in the vicinity that could possibly be another galaxy, however, the appearance of the main galaxy points to a low probability of any major merger events.
