The galaxy presents as a relatively smooth, elongated structure. It is characterized by a bright, concentrated central bulge that fades gradually into an extended, less luminous disk. The morphology appears to be intermediate between a flattened spheroid and a cigar shape. There is a suggestion of a disk component, but spiral arms are not clearly resolved in this image. The galaxy's color is consistent with a population of older stars, indicating ongoing star formation activity. There is no obvious evidence of major mergers or tidal disturbances affecting the galaxy's overall structure.
