This galaxy presents as an elongated, possibly edge-on or highly inclined spiral. It appears to have a concentrated central bulge region exhibiting a yellowish hue, suggesting an older stellar population and less active star formation within the core. Fainter, bluer extensions emanate from either side of the bulge, indicative of a disk component where younger stars and ongoing star formation may reside. The disk appears somewhat asymmetrical, possibly due to interactions or past minor mergers. A general smoothness in the overall light distribution is observed, but with hints of subtle irregularities within the disk, potentially reflecting faint spiral arm structures or dust lanes. The galaxy is moderately luminous, with a visual color that suggests a transitional stage between a blue star-forming spiral and a redder, quiescent elliptical.
