The galaxy presents as a moderately bright, elongated structure. Its overall morphology appears to be relatively smooth, with a subtle color gradient. The central region exhibits a slightly more concentrated yellowish hue, suggesting an older stellar population. This color gradually transitions to a fainter, somewhat bluer tint towards the outer edges of the galaxy, which may indicate the presence of younger stars or ongoing star formation, albeit at a modest rate. There appears to be little to no visible spiral structure. The galaxy's shape is notably cigar-shaped. No obvious signs of significant tidal disturbances or major mergers are apparent. The galaxy displays a well-defined structure, implying a settled state.
