The galaxy presents as a relatively compact, elliptical or lenticular system. Its morphology appears largely smooth with no obvious spiral arm structures or significant dust lanes visible in this image. The color profile indicates a redder hue, suggestive of an older stellar population and/or a higher abundance of dust within the galaxy. There is little evidence of active star formation based on the color and smooth morphology. The galaxy exhibits a high degree of central concentration, indicative of an evolved system dominated by older stars. There are no signs of ongoing major merger activity or significant tidal disturbances.
