The galaxy presents as a relatively small, faint object with an apparent smooth morphology. It appears elongated, exhibiting an elliptical shape rather than a well-defined spiral structure. There is no clear evidence of prominent spiral arms or a distinct central bulge. The color is somewhat uniform across the galaxy, with a slight indication of being redder in the core with bluer outskirts, suggesting a population of older stars dominating the central regions and younger stars present in the outer regions. There are no obvious signs of ongoing major merging activity, although subtle disturbances cannot be entirely ruled out based on this image alone. Based on its apparent size and lack of distinct features, this galaxy may represent a dwarf elliptical galaxy at intermediate redshift. Further spectroscopic analysis would be necessary to confirm the stellar population properties and determine its precise classification.
