The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a high degree of luminosity, appearing significantly brighter compared to the outer regions. The light is concentrated towards the center, diminishing gradually towards the edges, suggesting a centrally dominant stellar population. There is no evidence of distinct spiral arms, bars, or a well-defined disk. The galaxy appears largely symmetrical with a somewhat rounded morphology. There is no evidence of any major ongoing merger activity or significant tidal disturbances, although subtle asymmetry can be detected. The galaxy exhibits a yellowish-white hue, suggesting a population of older stars. The galaxy is roughly 5 kpc across. The overall appearance suggests a evolved system, potentially with a relatively low star formation rate.
