The galaxy appears to be relatively small, exhibiting a diffuse morphology. Its light profile suggests a smooth structure, with minimal evidence of distinct spiral arms or a prominent central bulge. The color index indicates the presence of a population of older stars, with an absence of significant star forming regions. Subtle, faint disturbances in the galaxy's outer regions are possibly indicative of minor gravitational interactions. The overall low surface brightness and smooth texture hint at a galaxy that may be a dwarf spheroidal or a highly-inclined disk galaxy with minimal recent star formation.
