The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, relatively featureless morphology. Its overall shape is elongated, being significantly wider than it is tall. A bright, concentrated central bulge or core is evident, gradually fading into a less luminous outer region. There is a subtle colour gradient observed, with the core showing a yellowish or orange hue, indicative of an older stellar population. The outer regions display a faint bluish tinge, which may signify the presence of younger, hotter stars. The structure appears largely undisturbed, with no visible signs of ongoing major mergers or tidal interactions. Faint patchy regions or dust lanes might be present, but this is uncertain due to the image resolution. The galaxy exhibits no clearly defined spiral arms. Its overall smooth appearance suggests a high fraction of spheroid stars.
