The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a dominant central bulge, characterized by a bright, yellow-orange hue, which suggests an older stellar population. There's a subtle falloff in intensity moving outwards from the core, with a less defined, fainter halo surrounding the central region. The overall structure lacks any prominent spiral arms or distinct features typically associated with disk galaxies. Based on the lack of strong blue colors, it's likely the galaxy exhibits a low star formation rate. There is no strong evidence of any ongoing major merger events, such as tidal tails or significantly distorted morphology, although there may be a subtle disturbance in its overall shape.
