The galaxy presents as a well-defined elliptical object, exhibiting a smooth, centrally concentrated morphology. The central bulge is characterized by a yellowish-gold hue, suggesting an older stellar population. Moving outwards from the core, the light gradually fades into a diffuse, bluish halo. The overall shape is elongated, appearing cigar-shaped, with a relatively high degree of symmetry. There are no readily apparent signs of spiral arm structures or significant dust lanes. The smooth, featureless appearance points towards a system dominated by evolved stars, with little active star formation occurring at the present epoch. There is a slight asymmetry in the extended halo, with one side appearing subtly more prominent. While seemingly isolated, closer analysis may be needed to determine if it had any minor gravitational disturbances.
