The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light distribution is relatively even, with a notable decrease in intensity moving outwards from the core. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a slightly rounded shape, appearing almost circular in projection. Faint indications suggest a possible minor disturbance in its gravitational environment, but no major merging events or significant tidal features are apparent. The color gradient suggests a population of older stars dominating the overall light output. The overall impression is that of a mature, relatively quiescent system.
