The galaxy presents as a relatively small, faint object. Its morphology is somewhat amorphous, lacking a well-defined spiral structure or elliptical shape. There appears to be a slight central concentration of light, possibly indicating a bulge. The color profile suggests a mixed stellar population, with some bluer regions potentially indicating ongoing star formation, while redder regions could indicate older stellar populations. There is a hint of disturbed features, which might indicate a past or ongoing interaction with another galaxy, or some other form of disruption. No clear signs of a major merger, though some minor disturbances could indicate some form of gravitational interaction.
