The galaxy presents a generally smooth and concentrated morphology, exhibiting a somewhat elliptical shape rather than a clear spiral disk structure. The light distribution is centrally concentrated with a bright, relatively small core that fades gradually outward. The color profile suggests a population of older stars, appearing more reddish-yellow, particularly within the central bulge. There is some slight indication of faint, diffuse features extending from the central region, but these are not well-defined spiral arms or distinct structures. The overall appearance is consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy, viewed at a moderate distance. There may be some minor interaction with other galaxies present, but this is difficult to confirm with the given image. Based on the observed properties, star formation is likely low, suggesting a predominantly older stellar population.
