The galaxy appears to be a relatively smooth, elliptical-type system. It exhibits a centrally concentrated bulge that dominates the light profile. The core is a bright, yellowish-white, gradually decreasing in intensity outwards. There's an apparent lack of prominent spiral arms or distinct disk structures. The galaxy's overall shape is generally rounded, though a slight elongation suggests it may not be perfectly spherical. There's no obvious evidence of significant tidal disturbances, major mergers, or ongoing star formation regions that would present with localized blue light. The color suggests a population of older stars.
