The galaxy presents a roughly elliptical morphology with a high degree of central concentration. The light distribution is smooth and appears relatively featureless. A subtle colour gradient is observed, with the central region exhibiting a yellowish hue, possibly indicative of an older stellar population, while the outer regions show a slightly bluer tint, suggesting the presence of younger stars or ongoing star formation. There is a faint extension of light along a particular axis. The overall impression is that of a relatively evolved galaxy with signs of potential minor disturbances.
