The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central region. It appears moderately luminous, with an overall yellow-orange hue. There is a possible indication of a secondary nucleus or merging event causing a slight distortion in its otherwise rounded form. No prominent spiral arms or dust lanes are immediately apparent in this image. The galaxy shows a color profile suggesting an older stellar population with reduced ongoing star formation. Slight tidal disruptions may be present that indicate recent or ongoing interactions with a smaller galaxy.
