The galaxy presents as a single, relatively smooth object with a somewhat elliptical morphology. The light distribution suggests a centrally concentrated structure, with a gradual decrease in surface brightness towards the outer regions. The galaxy appears to be a yellowish hue, with minimal evidence of strong blue star formation regions or prominent dust lanes. There are no immediately obvious signs of significant tidal disturbances or ongoing major merger activity. A slight asymmetry is noted in the light distribution, potentially indicating a minor interaction or internal feature. Based on its overall appearance, the galaxy likely represents a population of older stars and a modest amount of on-going star formation activity.
