The galaxy presents as an elliptical morphology, with a concentrated, luminous core that gradually decreases in intensity outwards. The central region exhibits a yellowish hue, suggesting a population of older stars. Surrounding the core is a fainter, more diffuse halo with a slightly bluer tint, which may indicate more recent star formation activity compared to the core. The overall shape is mostly round, though there's a slight elongation. There is no readily apparent presence of prominent spiral arms or a well-defined disk structure. No signs of ongoing major merger activity are visible. The general appearance suggests a relatively quiescent system with a dominant population of older stars.
