The galaxy appears as a centrally concentrated, elliptical-like structure. Its light profile indicates a relatively smooth distribution, with a high degree of central concentration, with a round shape. I do not observe any pronounced spiral arm structures, distinct bars, or evidence of significant tidal disturbances or ongoing major mergers based on the image. The color indices suggest a population of older stars is a likely source of the observed light, which points to low rates of current star formation. The galaxy's magnitude appears to be quite bright, suggesting a massive galaxy.
