The galaxy presents as a luminous, relatively smooth elliptical structure. It exhibits a bright, concentrated core region that gradually diffuses outwards into a less intense halo. The overall shape approximates a slightly elongated spheroid, appearing somewhat flattened, suggesting it may not be a perfect sphere. The color distribution shows a central region with a yellowish-white hue, indicating a population of older stars. Moving outward, the color shifts towards a bluer shade, suggesting the presence of a younger stellar population or ongoing star formation activity in the outer regions. There is no clear evidence of distinct spiral arms or significant dust lanes. The galaxy appears to be a relatively isolated system, showing no immediate signs of major gravitational interaction or tidal disturbances with other galaxies. Minor irregularities or subtle asymmetries may be present but are not immediately apparent.
