The galaxy appears to be an elliptical type, exhibiting a largely smooth, spheroidal morphology. The central region displays a concentrated luminosity profile, suggesting the presence of an older stellar population. There's a subtle color gradient observable moving outwards from the core, from yellower hues in the center to the color trending toward red in the halo. The color suggest a diminished presence of ongoing star formation, possibly indicating that the galaxy is relatively quiescent in its current evolutionary stage. There appears to be a slight tidal disturbance visible as a faint tail. This could be evidence of a past, or ongoing, minor galactic interaction.
