The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, with no obvious spiral arms or significant dust lanes visible in this image. The galaxy exhibits a moderate degree of roundness, appearing slightly elliptical rather than highly elongated. There are no immediately apparent signs of ongoing or recent major merging activity, although subtle disturbances cannot be ruled out at this resolution. The color index suggests the presence of an older stellar population, with a relatively low rate of current star formation. The overall luminosity is consistent with that of a moderately massive galaxy.
