The galaxy presents as a centrally concentrated, relatively smooth object with a high degree of roundness. The primary structure appears to be a spheroid with a bright, moderately compact core region that exhibits a warm hue. Extending from the core, a fainter, more diffuse halo is observed, contributing to the overall rounded appearance. There is some evidence of a subtle extension or tidal feature to one side, suggesting possible gravitational interaction or a past merger event. There is very little or no visible structure such as defined spiral arms or prominent dust lanes. The color profile suggests a population of older stars, indicative of relatively low current star formation activity. The galaxy lacks significant irregularities or strong disturbances in its overall morphology.
