The galaxy appears as an elongated, cigar-shaped structure. The central bulge exhibits a yellowish-white hue, indicative of an older stellar population. Extending outwards from the bulge are fainter, bluish-white regions, suggesting the presence of younger, hotter stars. The overall smoothness of the light distribution points towards a galaxy with a dominant spheroidal component. There is no clear spiral arm structure visible. The lack of strong dust lanes or prominent star-forming regions suggests a relatively quiescent galaxy. Faint irregularities in the outer regions may suggest minor past interactions, but no major mergers are apparent. The galaxy displays a color gradient, with the core being redder and the outer regions bluer, consistent with inside-out galaxy formation.