The galaxy presents as a relatively well-defined structure with a concentrated central bulge. This central region displays a yellowish hue, suggesting an older stellar population. Surrounding the bulge is a fainter, more diffuse disk component, appearing slightly bluish. The disk exhibits some irregularities, possibly indicating the presence of spiral arms or tidal disturbances. The overall morphology suggests a galaxy with a disk component that may be undergoing some form of interaction or internal rearrangement, deviating from a perfectly symmetric structure. The size appears moderate, neither exceptionally large nor compact compared to other galaxies in the field of view. The galaxy's color profile indicates ongoing star formation, although potentially at a moderate rate within the galaxy as a whole. There may be some evidence of minor interaction or disruption given the irregularities and faintness in the disk region.
