The galaxy appears as a single, centrally concentrated object with a smooth morphology, lacking any discernible spiral arm structures or prominent dust lanes. The light distribution suggests a spheroidal shape, appearing mostly round with some slight elongation. The color profile shows a dominant red-yellow hue in the core, transitioning to a greenish halo. This color gradient could suggest a population of older stars concentrated centrally with some ongoing star formation occurring in the surrounding area. There is a smaller, dimmer red object nearby which may be a satellite galaxy or a background object. There are no signs of significant tidal disturbances or ongoing major merger activity within the galaxy's visible structure. 
