The galaxy presents as a relatively compact object, exhibiting a generally smooth and rounded morphology. There's a noticeable concentration of light toward the center, suggesting a bulge component. While the overall structure appears smooth, closer inspection reveals faint, subtle features within the disk. The color distribution indicates varying stellar populations, with a bluer hue on the outer edges perhaps indicating ongoing star formation, while the central regions trend toward redder colors, possibly indicative of older, more evolved stars. There is no definitive evidence of significant spiral arm structure, a prominent bar, or any major tidal disturbances or interactions with other galaxies within the immediate vicinity. Some minor disturbances may be present. The galaxy is moderately luminous.
