This galaxy exhibits a smooth, elongated morphology, approximating a cigar-like shape. The light distribution appears relatively uniform, with no obvious spiral arms or distinct features. The central bulge is not clearly defined. The color gradient suggests a population of older stars, potentially indicating a relatively low current star formation rate. There is a slight hint of bluer light at the edges, which could indicate the presence of some younger stars or ongoing star formation. There is no evidence of any major mergers or significant tidal disturbances affecting its structure. The galaxy appears to be a relatively isolated system.