The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. The core region exhibits a bright, yellowish hue, suggesting an older stellar population. Moving outwards from the core, the color transitions to a bluer shade, which may indicate the presence of a younger, though still subdued, stellar population compared to typical star-forming galaxies. There is no visible spiral structure or prominent dust lanes. The galaxy's overall shape is generally round, with a slight elongation that could be described as moderately elliptical. There is no evidence of ongoing major merger activity, although subtle irregularities in the outer regions cannot be ruled out with the available image resolution.
