This galaxy exhibits a disk-like structure with an apparent bulge. The morphology suggests characteristics of both a spiral and an elliptical galaxy, potentially falling into the lenticular category. The spiral arms are not well-defined, appearing somewhat flocculent and disturbed, exhibiting a patchy distribution of light. These regions also have a slightly blue tint. The central bulge exhibits a yellowish hue, indicative of an older stellar population. Based on its irregular features, there may be signs of minor disturbances, possibly indicative of past or ongoing interactions. The light distribution is not uniform across the disk, indicating variations in stellar density and composition. The estimated size of this galaxy is roughly 5 kpc. While the bulge appears prominent, the disk contributes significantly to the overall luminosity. The estimated mass puts this galaxy in the lower end of normal. The estimated star formation rate for this galaxy is minimal.
