The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The luminosity profile appears to follow a Sersic model with a relatively high index, indicating a steep decline in brightness from the core outwards. The color distribution shows a general redder hue, characteristic of older stellar populations and lower star formation activity. There is a very slight flattening of the galaxy shape, suggesting a minor degree of ellipticity. Overall, the galaxy appears to be a relatively massive, evolved system with little evidence of ongoing mergers or significant disk-like structure.
