This galaxy presents as a relatively smooth, centrally concentrated object. There is a bright, diffuse bulge region exhibiting a slightly elongated, though not significantly cigar-shaped, form. A fainter, less distinct disk component surrounds the central bulge. There may be some possible disturbance, although this is subtle and could be due to image artifacts. The overall structure suggests a transitional morphology between elliptical and spiral types. The color profile indicates a redder core potentially indicative of an older stellar population, while bluer hues, though faint, in the outer regions possibly indicate ongoing or recent star formation.
