The galaxy presents as a largely smooth, elliptical structure. It appears to be mostly featureless, lacking any prominent spiral arms or bar structures. The central region exhibits a higher surface brightness, suggesting a concentrated nucleus. The overall shape is elongated, with the ratio of the major to minor axis being about 2 to 1. There is a slight distortion or faint plume extending from the upper right side of the galaxy, which may indicate minor tidal interactions or recent merger activity, but this requires further investigation. The color gradient suggests a population dominated by older stars, as indicated by the redder hues. There is very little evidence of active star formation from this image, the galaxy appears to be in a relatively quiescent state.
