This galaxy presents a primarily smooth and concentrated appearance, with a distinct central bulge. The morphology leans towards an elliptical or lenticular type, showing a lack of prominent spiral arms or significant disk-like features. The color distribution suggests an older stellar population dominating the bulge region, evident from its yellower to redder hue. There is evidence of a surrounding halo or envelope, exhibiting bluer colors, possibly indicating regions of more recent or ongoing star formation. The overall shape is somewhat elongated, but not extremely so, appearing more like a flattened spheroid. There appears to be no major ongoing merger activity or strong tidal distortions, although a slight asymmetry or minor disturbance cannot be ruled out. The galaxy seems relatively isolated, without any immediately apparent close companions or signs of strong gravitational interaction.
