The galaxy exhibits a central, moderately bright bulge region that appears yellowish-red in color, suggesting an older stellar population. Surrounding the bulge, there is a fainter, somewhat asymmetric disk component. A region of blue-ish light is visible on one side of the galaxy, indicating the presence of younger, hotter stars and possible ongoing star formation within that area. The overall morphology appears somewhat disturbed, possibly indicating a recent or ongoing interaction with another galaxy. The galaxy does not appear to be a classic spiral or elliptical, instead it seems to be in between. Some faint extended features are visible, hinting at tidal tails or disrupted structures resulting from the possible interaction.
