The galaxy presents as a relatively bright object with a concentrated central bulge and a flattened disk extending outwards. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. The disk appears somewhat dusty with subtle hints of spiral structure. The galaxy appears to be inclined significantly relative to our line of sight, nearly edge-on. The disk is elongated, with the major axis significantly larger than the minor axis, implying a substantial degree of flattening. There appears to be some disruption within the galaxy, possibly a minor merger event.