The galaxy presents as an elliptical or lenticular type, exhibiting a high degree of central concentration. Its light profile appears smooth, with no readily discernible spiral arm structures or prominent dust lanes. The color gradient suggests a relatively older stellar population dominating the galaxy's composition. The galaxy is elongated, with a clear major axis, suggesting that if it has a disk component, it is viewed at an oblique angle. The core is relatively small but very bright, with a softer halo surrounding it. There appears to be some minor interaction present as one side of the galaxy presents with a rougher edge. The colors present indicate the presence of different star formations, as well as the potential presence of an active galactic nucleus, contributing to the overall observed spectral energy distribution.
