The galaxy presents as a diffuse, elliptical-shaped object, exhibiting a centrally concentrated luminosity profile. It is characterized by a smooth, homogenous appearance, lacking any discernible spiral arm structures or prominent dust lanes. The color gradient transitions from a yellowish-white core to a fainter, redder halo, suggesting a stellar population dominated by older, redder stars. The morphological classification appears to lean toward an elliptical galaxy type, possibly an E4 or E5 based on the elongation. There is no evidence of active galactic nuclei activity or any significant ongoing star formation from the color and lack of distinct features. It does not seem to be undergoing any major merging events or tidal disturbances. The galaxy is a relatively isolated system.
