The galaxy presents a generally smooth morphology, with a high degree of central concentration. The primary body of the galaxy appears elliptical in shape, exhibiting a radial gradient in luminosity. The color profile is consistent with an evolved stellar population, displaying a yellowish hue indicative of older stars. There is a smaller, less luminous object located in close proximity to the primary galaxy, whose nature is currently unclear. It could be a globular cluster, a background galaxy, or a component of an ongoing interaction event, however, based on the data, it is unlikely that this galaxy is currently undergoing a major merger. Overall, the features suggest an elliptical galaxy that is relatively isolated. Further spectroscopic analysis is recommended to determine stellar population, gas content, and confirm the companion's nature.
