The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse morphology with no readily discernible spiral arm structure. The galaxy displays an elongated shape, with an approximate axis ratio indicating a moderate degree of flattening. The central region appears brighter and more concentrated than the outer regions, exhibiting a gradual decrease in luminosity with increasing radial distance. The color profile suggests a relatively old stellar population, dominated by redder wavelengths. There is no strong evidence of ongoing star formation. There is no apparent interaction with other galaxies.
