The galaxy presents as a relatively face-on spiral or lenticular system. The central region appears as a bright, diffuse bulge, characterized by a smooth distribution of light, suggesting an older stellar population. There is evidence of a faint, disklike structure surrounding the bulge, but any distinct spiral arms are subtle and lack clear definition. There is some indication of minor disturbances, possibly suggesting an ongoing or recent interaction or minor merger, as there appears to be some asymmetry in the distribution of light in the outer regions of the galaxy. The galaxy exhibits a blueish hue, with hints of redder colors at the edge of the galaxy, potentially suggesting active star formation, although subdued. Overall, the galaxy appears to be a moderately sized system with a combination of old and potentially some young stellar populations, with a hint of interaction.
