The galaxy presents as a thin, elongated structure, highly inclined with respect to our line of sight. Its disk appears relatively smooth with no discernable spiral arm features or bright knots of star formation visible in this image. There is a slight central bulge, appearing rounded and with no obvious boxy morphology. The galaxy exhibits a moderate luminosity across the observed spectral bands, with a redder color, indicating a population of older stars and/or significant dust extinction. There is no evidence of ongoing major mergers or strong tidal interactions. Faint, extended halos may be present, but confirmation requires higher resolution imaging.
