The galaxy appears as a single, relatively smooth object with a concentrated central region. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue. There is little evidence of spiral arm structure or significant dust lanes; the light distribution is largely uniform throughout the galaxy's body. Its overall shape can be described as rounded, lacking any elongated or irregular features. There are no indications of active star formation regions or tidal disturbances that would suggest recent merger activity. The galaxy seems well-defined and isolated, appearing as a single, coherent structure.
