The galaxy presents as a somewhat amorphous, diffuse structure with a dominant bluish hue. Its form appears to be transitioning, not clearly elliptical nor fully spiral. There's a central, brighter concentration of light suggesting a core region or bulge, but it lacks sharp definition. The galaxy exhibits faint extensions or tidal features, hints of possible past interactions or ongoing disturbances. The overall luminosity suggests a moderate stellar population, and the blue color indicates the presence of young, hot stars, implying current or recent star formation activity. However, its smoothed appearance suggests this activity may be subdued compared to more actively star-forming galaxies. Minor disturbances in morphology are visible but not significantly affecting the overall galaxy structure.
