The galaxy appears to be a smooth, elliptical system. Its color profile shows a dominant yellowish hue, with slight hints of red, suggesting a population of older stars and a relatively low rate of ongoing star formation. The shape is moderately elliptical, but it is generally elongated. There is no evidence of prominent spiral arms, dust lanes, or significant tidal disturbances, indicating that it has likely experienced minimal interactions or mergers recently. The galaxy is compact and centrally concentrated, with brightness decreasing gradually from the center outwards. 