The galaxy presents as a generally elliptical morphology, appearing largely smooth and featureless. It exhibits a high degree of central concentration with a bright, well-defined core that diminishes in intensity toward the outer regions. The observed color gradient suggests a population of older stars, particularly in the central bulge. There is no visible dust lane or prominent spiral arm structure. Faint, subtle irregularities might be present in the outer halo but are difficult to confirm. Overall, the galaxy appears to be a relatively quiescent system, not currently undergoing any major mergers or exhibiting strong star formation activity. Its estimated size would classify it as a galaxy of moderate size.
