The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core appears bright and somewhat diffuse, transitioning gradually into a more extended halo. Color gradients are subtle, with a slightly redder hue in the central region. There is minimal evidence of spiral arm structure. Overall, the galaxy appears relatively undisturbed, lacking prominent tidal features or evidence of a major ongoing merger event, however a possible minor disturbance is present in the asymmetry of the halo. The major axis appears to have a somewhat cigar-like shape with a moderate ellipticity. The overall size is moderate, suggesting this is a galaxy of substantial, but not extreme, physical dimensions. Based on its color and morphology, this object likely has a stellar population dominated by older, redder stars, and a relatively low ongoing star formation rate.
