The galaxy presents a generally smooth morphology. It appears as a relatively concentrated, centrally bright object with a significant bulge. The light distribution is largely elliptical, trending towards round, though with some subtle elongation that is difficult to fully resolve given the image quality. No distinct spiral arm structure is discernible; instead, the outer regions exhibit a diffuse glow that fades gradually into the background. There is no evidence of a major ongoing merger or significant tidal disturbances. The galaxy's color profile suggests a well-evolved stellar population, with yellow-red hues dominating the central bulge and more muted colors in the outer halo. Based on this analysis, the galaxy is most likely an elliptical galaxy, potentially of type E1-E3. There may be some low level star formation occurring, but it is difficult to determine with any certainty.
