The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, centrally concentrated light distribution, suggesting a relatively evolved system. The color profile indicates a yellowish core, transitioning to bluer hues in the outer regions. This color gradient might suggest older stellar populations are more centrally located, with younger, bluer stars residing in the outer areas of the galaxy. There is no clear evidence of spiral arm structure or significant dust lanes visible within the galaxy. The overall morphology points towards an elliptical or lenticular type galaxy. There are some hints of minor tidal disturbances or faint features, but these are not prominent and do not significantly disrupt the galaxy's smooth overall structure.
