The galaxy presents as an elongated, cigar-shaped system. The central region exhibits a concentrated luminosity profile with a yellowish hue, indicative of an older stellar population. Proceeding outwards, the galaxy transitions to a bluer, more diffuse disk. The disk structure appears relatively smooth, with no pronounced spiral arms or bar features visible in this image. There are hints of dust lanes along the equatorial plane, slightly obscuring the light. Overall, the galaxy appears to be an elliptical or lenticular system, possibly with a degree of ongoing, albeit low, star formation.
