The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The light distribution appears more or less even with no distinct features such as spiral arms immediately apparent. There is a slight elongation of the overall galactic shape; it is not perfectly circular, leaning towards an in-between shape. The color gradient suggests a population of older stars, giving it an overall yellowish to reddish hue. The central core is very bright, possibly indicating a high density of stars or an active galactic nucleus, though the limited resolution makes a definitive assessment challenging. There might be minor disturbances or interactions occurring, given the slight asymmetry observed, though the resolution constraints limit certainty on this aspect. The galaxy's overall form seems stable.