The galaxy presents as a relatively smooth, elliptical structure with an apparent lack of distinct features such as spiral arms or prominent dust lanes. Its overall shape is noticeably elongated, classified between round and cigar-shaped, suggesting a possible E4-E6 classification on the Hubble sequence. The color gradient indicates a higher concentration of older stars, particularly at the core. The central region exhibits a more intense yellow-orange hue, implying a population of evolved stars, while the outer regions appear slightly bluer, potentially indicating a lower level of ongoing star formation activity. There are no clear signs of a major ongoing merger or significant tidal disturbances. It appears as an isolated galaxy without any immediately apparent companions or strong gravitational interactions.
